The galaxy presents as a moderately luminous, early-type galaxy, likely an elliptical or lenticular. It exhibits a smooth, centrally concentrated light profile with a high degree of rotational symmetry. The galaxy appears somewhat spheroidal in shape, though a slight elongation is observed. The color gradient appears relatively uniform throughout, indicating a lack of significant recent star formation activity. The galaxy appears to have a fairly old stellar population. There is no obvious dust lane or disk structure visible. Furthermore, there are no readily apparent signs of tidal disturbances or ongoing major mergers. Subtle disturbances, such as faint tidal tails or a slight asymmetry in the outer isophotes, cannot be ruled out.
