The galaxy presents as a single, well-defined object with a smooth and rounded morphology. There are no discernible spiral arms or a distinct disk structure. The light distribution appears centrally concentrated, gradually fading towards the outer edges. The color is predominantly yellowish-orange, suggestive of an older stellar population with fewer young, hot stars. There is no evidence of significant tidal features or ongoing mergers. The lack of prominent blue regions indicates a relatively low rate of current star formation activity. The overall appearance suggests an elliptical galaxy, likely of substantial mass.
