The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge, suggesting a high density of stars in the core region. There is a slight elongation in its overall shape, leaning more towards an in-between roundedness. A faint disk is suggested, though not prominent. There is no obvious indication of any major ongoing merger activity or significant tidal disturbances, suggesting the galaxy is relatively undisturbed. Colors suggest old stars, indicating a population of redder stars. Star formation rate is assumed to be low. It has an overall smooth and regular appearance.
