The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge that displays a yellow-orange color. This suggests a population of older stars dominating the core. Moving outward from the center, the light gradually fades, exhibiting a slightly bluer hue. While a definite disk structure is not clearly visible, there is some indication of a flattened shape as opposed to being perfectly spherical. There are no strong indications of any major disturbances or ongoing mergers, such as tidal tails or distorted morphology, though there may be minor asymmetries within the galaxy. The relatively smooth appearance with a dominant bulge component suggests that star formation is either minimal or occurring at a low rate, consistent with a more evolved galaxy.
