The galaxy presents as a single, largely homogenous object. It exhibits a generally elliptical morphology, appearing mostly round in projection. The light distribution is centrally concentrated, with a smooth gradient outwards from the core. The galaxy's color profile indicates an older stellar population, with a yellowish-red hue dominating the observed light. There is no discernible evidence of spiral arm structure or significant dust lanes. Minimal signs of tidal disturbances or ongoing mergers are visible, suggesting a relatively quiescent evolutionary state. The galaxy appears to be a typical early-type galaxy with characteristics of an elliptical galaxy.
