The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. It is primarily characterized by a bright, roughly circular core region which appears to be quite compact. A slight extension or subtle asymmetry may indicate the presence of a weak disk-like structure, however this is not clearly defined. The overall color gradient suggests a higher concentration of older stellar populations, particularly toward the central region, implying a diminished current star formation rate. There is a potential indication of a very minor disturbance in the galaxy's structure. The galaxy is fairly isolated with no strong indications of a major merger event.
