The galaxy presents as a smooth, elliptical-like structure, with a concentrated central bulge that exhibits a yellowish hue, suggesting an older stellar population. There is a subtle color gradient emanating outward from the core, gradually fading into a redder, less luminous halo. No spiral arm structures are discernible. The galaxy appears to be isolated, showing no obvious signs of tidal interactions or ongoing mergers. It does not have an extremely round morphology but is not cigar-shaped either. Overall, it is a quiescent system.
