The galaxy presents as a single, relatively smooth, and concentrated object. It appears generally elliptical in shape, though slightly oblong, with the longer axis diagonal across the frame. The light distribution is centrally concentrated, showing a smooth fall-off in intensity from the core outwards. There is a hint of a faint disk or outer structure, though the overall appearance remains dominated by a smooth, spheroidal component. There is no apparent spiral structure nor strong evidence of recent or ongoing mergers. Color-wise, the central region exhibits a yellow-orange hue, suggesting an older stellar population, with bluer colors more represented on the outer edges, indicative of ongoing star formation. Overall, the galaxy appears to be a reasonably massive and somewhat evolved system, but with some signs of continued activity.
