The galaxy presents an overall smooth morphology, appearing largely featureless without prominent spiral arms or a well-defined disk structure. The object exhibits a roughly elliptical shape, tending towards being round. There is a concentration of luminosity towards the center of the galaxy, suggesting the presence of a galactic bulge. Color gradients are subtle, with a slightly more yellow or white core region that fades to bluer hues in the outer regions. This color distribution may imply older stellar populations concentrated towards the center, and younger, star-forming regions in the periphery. There is no clear evidence of ongoing major merging events or significant tidal disturbances from the galaxy's morphology.
