The galaxy appears as a single, centrally concentrated object. Its light profile is smooth and generally elliptical in shape, with a high degree of central concentration. There is little to no evidence of spiral arms or a distinct disk structure from this perspective. Color gradients are subtle, with a slightly redder central region, suggesting an older stellar population. No signs of strong tidal disturbances, ongoing mergers, or active star formation regions are visible. The galaxy exhibits a regular, relatively undisturbed morphology. The overall impression is that of a mature, early-type galaxy.
