This galaxy appears to be a relatively smooth elliptical galaxy with a high degree of central concentration. It exhibits a generally spheroidal shape. The galaxy displays a yellowish-orange hue, indicating a population of older stars with minimal ongoing star formation. There is no apparent spiral arm structure or dust lane features.

Based on visual assessment, it appears undisturbed, without obvious signs of tidal interactions or mergers with other galaxies, although there is the possibility of a merger remnant near the center of the galaxy.
