The galaxy presents as a relatively bright, extended object with a smooth, diffuse morphology. Its color appears to be primarily yellowish-white, suggesting a population of older stars with lower rates of star formation, or significant dust reddening. The galaxy has a roughly elliptical shape, appearing nearly round rather than highly elongated. There is a subtle hint of a possible minor disturbance in the galactic structure. There is no readily apparent spiral arm structure, and there is a lack of bright, blue regions indicative of ongoing star formation. The galaxy may be undergoing, or has undergone, a minor merger event.
