The galaxy presents a generally smooth and centrally concentrated morphology. The light distribution appears relatively even, with a slight elongation. The central region exhibits a yellowish-orange hue, which may indicate a population of older stars, or significant dust obscuration. Faint extensions, perhaps indicative of a weak disk or tidal features, are tentatively observed. The overall color profile suggests a galaxy transitioning from actively star-forming to a more quiescent state. There is no obvious presence of spiral arms or a prominent bar structure. The galaxy's shape appears closer to an elliptical than a spiral, though its exact classification is difficult to determine at this resolution. No signs of on-going mergers or tidal interactions are visible.
