The galaxy appears as a single object, but appears to be in the process of a merger. It presents with a relatively smooth, elliptical morphology. A small portion of the galaxy appears to be relatively circular, while the major section seems more elongated. The primary body has a yellowish hue, with a secondary object on one side that displays more red in its color. This red component suggests a higher concentration of older stars or dust obscuration. There is some indication of a slight disturbance in the overall structure, consistent with ongoing or recent gravitational interaction. The relatively smooth appearance with a dominant central bulge and the apparent lack of well-defined spiral arms suggests the galaxy has a relatively low rate of star formation. Overall the general appearance is one of a massive object. 
