The galaxy appears to be a relatively compact object. It displays a generally smooth morphology. There is no discernible disk component or spiral arm structure visible. A very faint suggestion of tidal distortion is present. The galaxy is not strongly dominated by a central bulge. The observed color suggests a higher proportion of older stellar populations, potentially indicating a lower rate of on-going star formation. The object does not seem to be undergoing a major merger. It presents an elliptical shape.