The galaxy appears as a concentrated, elliptical-like structure with a smooth, diffuse light profile, suggesting a relatively old stellar population. The central region is brighter and more condensed compared to the outer regions, which gradually fade into the background. The galaxy has a yellowish hue, indicative of a lack of recent star formation and the dominance of older, redder stars. There is no visible spiral arm structure or dust lanes, further supporting the classification as an early-type galaxy. Minor asymmetry is present; likely, the galaxy is undergoing a merger with a small dwarf galaxy. Overall, the morphology suggests a galaxy that has largely completed its star formation and is relatively quiescent.
