The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, diffuse morphology, lacking defined spiral arms or a prominent disk. The central region appears brighter and more concentrated. The color profile suggests a population dominated by older stars, indicated by the yellowish-red hue. There is no apparent evidence of significant dust lanes or active star-forming regions within the galaxy itself. There is no obvious tidal debris or disruption, suggesting the galaxy is relatively undisturbed by recent major interactions.
