The galaxy presents as a moderately bright, somewhat compact object with a generally elliptical morphology. It appears relatively smooth with a concentrated central bulge that is yellowish-white in color, indicating an older stellar population. The outer regions exhibit a bluer hue, suggesting the presence of younger stars or ongoing star formation, albeit at a lower rate. There is a subtle disk structure visible, though it is not particularly well-defined. There are no obvious signs of major disturbances such as tidal tails or significantly asymmetric features, though there may be very minor distortions in the outer regions that suggest some interaction history. No active galactic nucleus is readily apparent. Overall, the galaxy appears to be a relatively quiescent, intermediate-mass system with a mix of stellar populations.
