The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that transitions smoothly into a surrounding, less dense halo. There is a slight elongation, suggesting an elliptical shape rather than a perfect sphere. Color gradients are subtle but noticeable, with the core appearing more yellow, potentially indicating an older stellar population. A faint greenish hue exists in the outer regions, which could be associated with younger stars, or potentially ongoing, but subdued, star formation within a disk feature. There appears to be no evidence of strong tidal disturbances, merging activity, or distinct spiral arm structures. The galaxy likely resides at a considerable distance, indicated by its small angular size.
