The galaxy presents a generally smooth and rounded morphology. It displays a concentrated central bulge, which appears bright and yellowish-white, likely indicating a population of older stars. The outer regions of the galaxy exhibit a more diffuse and fainter halo, transitioning to a bluer hue suggesting the presence of some younger stellar populations. There is little to no visible structure such as spiral arms or dust lanes, indicative of an elliptical or lenticular galaxy type. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, although minor asymmetries cannot be ruled out given the image resolution. Its relatively compact size and concentrated light profile suggest a galaxy that has largely ceased active star formation.
