The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. Its overall shape is generally round, with minimal deviation from circular symmetry. A bright, well-defined central bulge dominates the luminosity profile, suggesting a high concentration of older stars. The light is yellowish, implying an older stellar population with low star formation. There is no visual evidence of distinct spiral arms or a pronounced disk structure. Subtle color variations can be observed, with the core of the galaxy appearing yellower than the outer regions. There is no obvious signs of ongoing major mergers or tidal disturbances, though very faint asymmetries might indicate minor interactions.
