The galaxy presents as a generally smooth, elliptical-like structure, with a concentrated central bulge. It exhibits a moderate degree of ellipticity, appearing more elongated than perfectly spherical. The light profile seems to fade gradually from the core outward. The color gradient appears to be fairly consistent across the galaxy, trending towards redder hues, suggesting an older stellar population. There is a hint of a disk-like structure, but it is not particularly pronounced. No major disturbances are apparent in its morphology; there's no evidence of tidal tails or ongoing major mergers. Based on its appearance and overall color, the galaxy is likely a relatively massive system with suppressed star formation.
