The galaxy presents as a relatively smooth, centrally concentrated object with a predominantly elliptical morphology. There is no prominent disk structure or spiral arm features discernable. The light profile suggests a relatively even distribution, although the central region appears slightly brighter and exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions of the galaxy have a bluer tint, which could be indicative of more recent star formation, though the overall fraction of recent star formation appears to be small. The galaxy appears largely undisturbed, showing no clear signs of major merging events or tidal interactions. There is a very subtle, faint asymmetry that could indicate a minor interaction. Overall, the galaxy seems to be an evolved system, dominated by an older stellar population but with some ongoing, low-level star formation.
