The galaxy presents as a relatively compact object, elliptical in overall shape. The light distribution appears centrally concentrated with a bright, unresolved core. A disk-like structure appears to surround the central bulge. The colour profile of the galaxy indicates that it is bluer towards the edges and centre and redder away from the middle of the galaxy. Faint, extended features are discernible, potentially indicating a minor tidal interaction. The overall structure suggests the possibility of a past merger event or internal dynamical disturbance.
