The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color profile suggests an older stellar population, with a yellowish-red hue dominating. There is a slight elongation, although the galaxy is mostly round. Faint extensions from the main body of the galaxy could be minor disturbances, or tidal features, but no strong evidence of a major merger is apparent. No prominent spiral arms or distinct dust lanes are observed. A small amount of blue may suggest some regions of active star formation.