The galaxy presents as a relatively smooth, elliptical-shaped structure. It exhibits a concentrated central bulge that graduates outwards into a fainter halo. The color profile indicates an older stellar population, with a yellowish-red hue dominant across the galaxy. There is no apparent spiral structure or active star forming regions. No strong tidal features, mergers or disturbances are observed, suggesting the galaxy is isolated and has not undergone significant interactions recently. The general appearance is consistent with an early-type galaxy with high spheroidal component.
