The galaxy presents as a centrally concentrated, elliptical-like structure. There is a bright, diffuse core region with a gradual falloff in luminosity towards the outer edges. The galaxy exhibits a generally smooth appearance. There are no distinct spiral arms or significant dust lanes visible. The color profile suggests a relatively evolved stellar population. The galaxy shows a slight tilt relative to our line of sight, its shape is close to circular. The overall morphology suggests a galaxy that has undergone significant merging and relaxation processes.
