The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge and a gradual decrease in luminosity towards its outer regions. The overall color profile suggests an older stellar population, indicated by the yellowish hue, potentially devoid of significant recent star formation. The galaxy displays a nearly round shape, showing no obvious signs of a disk structure or spiral arms. There's no immediate visual evidence of ongoing major mergers or tidal disturbances. Some slight color variations across the galactic body might indicate subtle differences in stellar populations or dust distribution. The galaxy's spatial extent is fairly compact, suggestive of a moderate physical size.
