The galaxy presents as a single, largely featureless object. It exhibits a smooth, elliptical morphology with a high degree of central concentration. A gradual decline in surface brightness is observed moving outwards from the core. The galaxy appears roughly circular in projection, showing no obvious signs of strong tidal interactions or major morphological disturbances. Faint colour variations suggest the presence of underlying stellar populations with differing ages and metallicities, with the central regions appearing more homogenous in colour. There is a faint red halo visible indicating older stars on the outskirts of the galaxy. The overall light distribution is dominated by a smooth, centrally concentrated component.
