The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge which transitions into a more diffuse halo, suggesting a lack of significant recent star formation. The color profile indicates the presence of an older stellar population. The galaxy shows no obvious signs of spiral arm structure or significant dust lanes, reinforcing the conclusion that this is an elliptical galaxy. There is no indication of any major interaction or merging events. The galaxy has a fairly high degree of roundness, with no apparent distortions or elongated features. There is very little evidence of active star formation. 
