The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a bright, concentrated central bulge that gradually fades into the outer regions. Its overall shape is noticeably elongated but predominantly rounded. There is no obvious dust lane or spiral arm structure discernible. The color gradient suggests a stellar population that is predominantly older, with a yellow-orange hue dominating the central bulge and slightly bluer tones becoming visible in the surrounding halo, indicating a possibility of a small amount of recent star formation. There are no signs of major disturbances or tidal features which would be indicative of a recent major merger.
