The galaxy presents as a smooth, centralized object with an elliptical morphology. The light distribution is concentrated towards the center, indicative of a higher stellar density in the core region. There are no apparent spiral arms or distinct disk-like structures visible. The overall color is reddish-orange, suggesting a stellar population dominated by older, redder stars and a lower rate of ongoing star formation. There might be some very minor irregularities in the outer regions, but there are no strong indications of tidal features, recent mergers or major disturbances, with a somewhat round shape. The galaxy shows evidence of significant mass, considering the stellar population is slightly massive, while also having a very low specific star formation rate. The galaxy appears to be a somewhat isolated system in a late stage of its evolution.
