The galaxy presents a primarily smooth morphology. There is a slight asymmetry with a subtle extension or possible tidal tail feature emerging from one end. The main body of the galaxy exhibits a concentrated bulge or core region, which appears yellowish-orange in color suggesting a population of older stars. The galaxy's outer regions display a bluer hue, potentially indicative of ongoing or recent star formation. Given the smooth appearance, it is likely an elliptical galaxy, or potentially a spiral galaxy viewed at an angle that obscures any spiral structure. There is no obvious evidence of significant ongoing merger activity or major disturbances, but the slight asymmetry and possible tidal feature may suggest past interactions or minor disturbances. The general shape is neither perfectly round nor highly elongated.