The galaxy presents as a relatively smooth, centrally concentrated object with a moderate degree of roundness. The light distribution appears fairly uniform, lacking prominent spiral arms or a distinct bar structure. There is a slight elongation observed, though the object doesn't appear highly flattened. No signs of major mergers or significant tidal disturbances are immediately apparent, although subtle irregularities can not be excluded at this resolution. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in the central region to a redder color in the outskirts. The overall color suggests a population dominated by older stars, with the potential for some ongoing star formation within the core.
