The galaxy presents as a somewhat spheroidal object with a concentrated central bulge that is bright in the blue wavelengths. The concentration of light indicates a high stellar density. The central bulge is surrounded by a ring-like structure that appears as a mix of green and red. The morphology suggests that the galaxy is likely undergoing or has recently undergone some type of interaction or disturbance, evidenced by the disturbed outer regions with non-uniform light distribution. There is some evidence of faint tidal features extending outwards from the main body, but these are not well-defined.
