This galaxy presents as a relatively compact and luminous elliptical system. It appears to be largely spheroidal, with a smooth, featureless profile, but subtle irregularities are visible. There is an indication of a possible tidal interaction or minor merger event occurring, seen as asymmetry in the outer regions. The central bulge is dominant, displaying a yellowish-orange hue indicating an older stellar population, suggesting minimal ongoing star formation activity. The overall color is redder, indicating the presence of older stars with a high concentration towards the center. The galaxy lacks defined spiral arm structures or a prominent dust lane. There appears to be a companion galaxy in close proximity with similar characteristics to the primary galaxy, indicating the galaxy exists in a group. There is a very slight distortion in the morphology suggesting a merging event may be occurring.
