The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards. There is a yellow/white hue, suggesting a population of older stars. There may be a slight hint of blue in the outer regions. The galaxy exhibits little to no visible spiral arm structure or prominent dust lanes. There is no distinct nucleus visible, but that may be related to the image quality. The shape is mostly in between round and cigar shaped, but closer to round. No major merging or disturbance is visible, but it may be undergoing a minor disturbance. It appears to have a log stellar mass of approximately 10.7 to 10.8.