This galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. The central region appears bright and yellowish-white, indicating a population of older stars. The light smoothly decreases in intensity outwards to a lower surface brightness, diffuse halo. There is no clear presence of spiral arms, dust lanes, or other distinct features associated with ongoing star formation. The overall shape appears to be moderately elliptical, though not cigar-shaped. There is no visual evidence of tidal disturbances or ongoing mergers, although some very minor asymmetry cannot be entirely ruled out. Overall, the galaxy exhibits characteristics of a relatively quiescent system.
