The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, indicative of an older stellar population. A bluer, more diffuse halo surrounds the core, possibly suggesting some ongoing, albeit low, star formation activity in the outer regions. The galaxy appears relatively undisturbed, without any major signs of tidal interactions or ongoing mergers. The shape is somewhat elongated, with a slight cigar-shaped appearance. Overall, the galaxy seems to be a relatively isolated system with a dominant spheroidal component.
