The galaxy presents as an elliptical, or potentially lenticular, structure. It appears to be relatively smooth in texture, with a centrally concentrated luminosity profile and extended, albeit faint, outer regions. The light distribution suggests an aging stellar population. The galaxy seems to be undergoing, or to have recently undergone, a significant merger event with a smaller companion galaxy, which is visible in the foreground. There are no obvious spiral arm features, although it is possible that a faint disk component is present within the central regions. There does not appear to be much ongoing star formation in the main body of the galaxy, as there are no bright blue clusters of stars. The smaller foreground galaxy is much brighter, and may be a more actively star-forming galaxy.