The galaxy presents as a moderately luminous object with an apparent size suggestive of a galaxy at an intermediate distance. The overall morphology appears to be that of a disturbed system, possibly resulting from an interaction or merger. A bright, centrally concentrated bulge is evident, but it appears asymmetric, with an extension or tidal tail of diffuse material emanating from one side. The main body exhibits a smooth, relatively featureless structure, indicating an older stellar population. There are no discernible spiral arms. Overall, the galaxy's light is fairly red in color. The disturbed structure may be due to an ongoing or recent merger event with another galaxy.