The galaxy presents as a relatively smooth object, exhibiting a largely elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity outward from the core. The galaxy’s color profile indicates a redder hue, suggesting a stellar population dominated by older stars. The galaxy appears to be quite massive, with a very low rate of star formation. The overall impression is that of a well-formed, settled galaxy without significant ongoing mergers or tidal disturbances and appears relatively round. 
