The galaxy presents as a relatively compact, elliptical-type system. The light profile appears smooth and centrally concentrated, exhibiting a high degree of circularity. There is no discernible disk structure or spiral arm morphology. The color is predominantly yellow-orange, suggestive of an older stellar population with limited ongoing star formation. There is no indication of any major mergers or significant tidal disturbances affecting the galaxy's overall structure, nor is there visual evidence of an active galactic nucleus. The light output suggests it is a moderately luminous galaxy.
