The galaxy appears to be a relatively smooth, elliptical-type galaxy with a high degree of central concentration. The light distribution suggests a mostly featureless structure, with a gradual decrease in surface brightness from the core outwards. There's a slight elongation in the galaxy's shape, although it is predominantly round. Based on its morphology, it likely has a low star formation rate and a substantial stellar mass. The red color indicates an older stellar population. There is no evidence of tidal tails or major disturbances.