This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. The light distribution appears quite even, with no obvious spiral arm structures or significant dust lanes visible. There are hints of bluer tones at the outer edges, suggesting the possibility of some younger star formation regions, but the overall color is indicative of an older stellar population. The galaxy has a slightly elongated shape but is mostly in between round and cigar shaped. There is no major or minor disturbances occuring. 
