The galaxy appears to be a relatively smooth, elliptical-like structure. The core is bright and concentrated, with a gradual decrease in luminosity extending outwards. There is some evidence of a possible disk but it is not very prominent. It does not appear to be undergoing a major merging event, though some minor tidal disturbance cannot be ruled out. The overall color appears to be dominated by older stellar populations, giving it a slightly reddish-yellowish hue, with some bluer regions present as well. The object does not display a well-defined spiral structure.
