The galaxy presents as a fairly symmetrical, elliptical-like structure with a smooth light distribution, exhibiting a concentrated central bulge. The primary color gradient transitions from a yellowish-white core to a reddish-yellow outer region. This suggests a stellar population dominated by older stars, particularly in the bulge. No distinct spiral arms or prominent dust lanes are observed within this optical imagery. The lack of blue color suggests relatively low ongoing star formation. There may be some evidence of a slight tidal disturbance on the upper right edge of the galaxy.
