The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated luminosity profile. It exhibits a dominant, near-spherical morphology with a slight elongation along one axis. The color appears reddish-orange, suggestive of an older stellar population and reduced star formation. There may be some faint evidence of a disturbed morphology, possibly due to a minor interaction or past merger event. The main body is surrounded by a faint halo of diffuse light, which may indicate tidal debris or a population of older, more dispersed stars. The system shows low star formation.
