The galaxy presents as a moderately bright, relatively smooth elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright, unresolved core that gradually fades into the surrounding halo. The overall shape is more lenticular than spherical. The galaxy appears yellowish to white in color, suggesting a population of older stars. There is no strong evidence of spiral arm structure or significant dust lanes visible in the image. Faint irregularities along the outer edges of the galaxy indicate possible interactions with a smaller galaxy. This galaxy has a low star formation rate.
