The galaxy presents as a moderately bright, elliptical structure. Its light is centrally concentrated, exhibiting a smooth, diffuse profile. The nucleus appears unresolved, displaying a slightly bluer color than the surrounding halo. The halo itself fades gradually into the background, with no distinct features such as spiral arms or a prominent disk visible. There's no strong evidence of recent or ongoing major merger activity, though some subtle irregularities in the outer regions may suggest a minor interaction or past disturbance. Overall, this appears to be a relatively quiescent galaxy, likely dominated by an older stellar population. Its shape falls somewhere between round and elongated. The colors suggest a relatively low star formation rate.
