The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. There is a subtle color gradient from the core outwards, shifting from a yellowish-orange to a greenish hue in the outer regions. No prominent spiral arms or distinct dust lanes are apparent. The galaxy appears relatively isolated with no obvious signs of tidal interactions or ongoing mergers, although a very slight asymmetry may indicate a past minor interaction. The overall morphology suggests an evolved system with a relatively low star formation rate.
