The galaxy presents as a relatively compact object with an elliptical morphology. It exhibits a smooth light distribution, with a dominant central bulge. The galaxy's color appears to be generally redder, suggesting an older stellar population and potentially lower ongoing star formation. There is a slight asymmetry in the light distribution, possibly hinting at a minor interaction or internal disturbance. The overall structure appears relatively undisturbed, with no prominent tidal tails or signs of a major merger event. The galaxy's visual characteristics suggest it is a mature system, likely with a considerable stellar mass.
