The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. The light distribution indicates a high degree of radial symmetry. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy's color appears to be yellowish-white, suggesting a stellar population dominated by older, evolved stars. The lack of blue light implies relatively low current star formation activity. There are no indications of tidal tails or other morphological disturbances suggestive of recent or ongoing merger events. A slight color gradient is visible, with the core appearing slightly more yellow, and the outer region tending towards whiter hues. This could potentially point to metallicity differences or age variations in the stellar populations with the inner regions of the galaxy having older stars. The galaxy exhibits a relatively compact appearance, implying a high stellar density and/or that it is a smaller sized object. 
