The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a roughly elliptical shape, approaching circularity. The color profile suggests a dominant population of older stars, indicated by its redder hue. There are no clearly defined spiral arms or prominent dust lanes visible. There is some suggestion of minor disturbances in the symmetry of the outer regions, hinting at potential past interactions or mergers, but the overall structure is largely undisturbed. The galaxy's size is relatively substantial, implying a considerable stellar mass.
