The galaxy presents as a somewhat elongated structure with a brighter, seemingly unresolved central region, possibly indicative of a galactic bulge or active galactic nucleus. The overall color gradient suggests a mix of stellar populations. The central region exhibits a predominantly yellowish-white hue, which could imply an older, more evolved stellar population.

Extending outward from the center, there appears to be some disklike morphology with regions of bluer light, particularly at one end of the galaxy. These bluer regions likely indicate areas of ongoing or recent star formation, where hotter, younger stars are more prevalent. Additionally, there's a slight reddish area at the opposite end, possibly representing another site of star formation or older stellar populations reddened by dust.

There appears to be some disturbances in the galaxy's structure; it is somewhat asymmetrical. These disturbances could potentially be indicative of past interactions with other galaxies, though no clear signs of an ongoing major merger are immediately apparent in this image alone. The galaxy's overall structure could suggest a transitionary stage between a spiral and elliptical morphology, or perhaps a galaxy that has undergone some type of interaction that has perturbed its shape. Further investigation with higher resolution imaging and spectroscopic data would be necessary to fully characterize its morphology and evolutionary history.
