The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, bright central region with a diffuse halo extending outwards. The galaxy presents a generally rounded shape. There is a noticeable color gradient, shifting from a yellowish-white core to a more reddish hue in the outer regions. No significant spiral arm structures or distinct dust lanes are discernible. There is no obvious evidence of a major ongoing merger or tidal disruption. The galaxy's overall morphology suggests a relatively evolved system with a dominant bulge component and minimal recent star formation activity. Minor irregularities in the outer halo could indicate past interactions.
