The galaxy presents as a single, centrally concentrated object. Its overall morphology appears smooth, lacking any prominent spiral arms or distinct disk-like features. The light distribution suggests a radial profile, with the highest intensity located at the core, gradually decreasing towards the outer edges.

The galaxy's color is relatively uniform, exhibiting a general yellowish-white hue with a slight red tone, implying a stellar population dominated by older stars with suppressed recent star formation. The shape leans toward being somewhat rounded. There are no obvious signs of tidal disturbances or ongoing major merger activity. Subtle color variations could imply mild disturbances or low-level merger.
