The galaxy appears to be a relatively smooth, elliptical type. Its overall shape is somewhat flattened but not distinctly disk-like. A bright central bulge dominates the galaxy's structure, fading gradually into the outer regions. The color is predominantly yellow-orange, suggesting an older stellar population with fewer hot, young stars. Some evidence of minor disturbances or asymmetries can be inferred, possibly indicative of past interactions or mergers. However, there isn't a very clear indication of strong tidal tails or prominent merger features. There are no signs of active star formation. The lack of dust lanes is noticeable. It is likely a massive galaxy.
