The galaxy presents as a slightly elongated, diffuse object. Its overall structure appears relatively smooth, with a concentrated central bulge that dominates the light profile. The light from the galaxy spans a few kiloparsecs. There are faint indications of a disc, but no clear spiral arm structures are visible. The galaxy's core emits light predominantly at the green-yellow end of the spectrum, with this region appearing somewhat unresolved in the available image. There are hints of redder emission extending outwards from the central bulge, indicating potentially older stellar populations in the outer regions. The shape of the galaxy is in between round and cigar-shaped, which may indicate it is either an elliptical galaxy, or a face on spiral galaxy. There does not seem to be evidence for strong star formation activity in this image. The galaxy's appearance suggests a relatively evolved system. There may be a minor disturbance.
