The galaxy appears as a moderately bright, elliptical structure with a smooth, diffuse morphology. The light distribution indicates a centrally concentrated luminosity profile. The galaxy exhibits a color gradient, transitioning from a bluer central region to redder outskirts. This suggests younger stellar populations are more concentrated toward the center, with older, redder stars dominating the outer regions. Although the galaxy shows a general elliptical shape, there is a subtle hint of a disk-like structure embedded within. No significant tidal features or prominent dust lanes are visible. Overall, the galaxy seems to be a relatively undisturbed system with ongoing, albeit potentially low, star formation occurring primarily in its core. The estimated size is approximately 4 kpc.