The galaxy appears to be elliptical in morphology, exhibiting a generally smooth light distribution. The core region shows a high degree of symmetry, becoming less homogenous towards the outer edges, suggesting possible interaction with other bodies. The overall color of the galaxy is skewed toward redder wavelengths. There is not obvious presence of spiral arms or a prominent disk-like structure. There is a very faint disturbance on the left side that may be due to gravitational disturbance, perhaps in the early stages of a possible merger event or interaction with a smaller body.
