The galaxy presents as an elliptical or lenticular type. The light distribution is centrally concentrated, diminishing outwards with a gradual decrease in intensity. The object exhibits a relatively smooth profile, showing only subtle irregularities in its overall structure. A slight elongation is observed, with the galaxy appearing more oval than perfectly spherical. Hints of bluer colors are seen towards the edges and may suggest some recent star formation. While there is no dominant spiral arm structure, the object is not entirely homogenous and shows some minor disturbances. Overall, the galaxy appears to be a mature system with a significant population of older stars.
