The galaxy presents as a relatively compact structure. Its overall form appears elliptical, tending towards a prolate spheroid. The light distribution indicates a smooth profile, with minimal discernible substructure. However, there is some suggestion of minor tidal disturbance or interaction, hinted by subtle asymmetries in the outer regions, potentially from a past merger or ongoing interaction. The core exhibits a somewhat diffuse appearance. There may be the suggestion of some dust obscuration or patchy star formation.
