The galaxy presents as a relatively smooth, elliptical-like structure. Its core is characterized by a bright, concentrated region, suggestive of a high stellar density, possibly an active galactic nucleus, or both. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes within the resolution limits of the image. There is a subtle color gradient, with the central region exhibiting a more yellow hue, potentially indicative of an older stellar population compared to the outer regions, which appear slightly bluer. The galaxy's profile suggests a generally round shape. There are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity. The overall morphology indicates a well-evolved system dominated by a smooth, spheroidal component.
