The galaxy presents as a fairly smooth, elliptical-like structure. It appears to have a concentrated central bulge region exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions exhibit a slight blueish tint and appear less concentrated than the central bulge, suggesting the presence of some younger stars or ongoing star formation. The overall morphology indicates a relatively relaxed system with a possible lack of recent major merger activity, although there may be some minor asymmetry or tidal features that need further investigation.
