The galaxy presents a generally smooth and rounded morphology, appearing as a single, cohesive unit. It is characterized by a concentrated central region that appears brighter and more luminous than the surrounding areas. There is very little visible evidence of spiral arm structure or distinct features typically associated with disk galaxies. The galaxy exhibits a color gradient, appearing yellowish in the center and gradually shifting to a redder hue towards the outer edges. There are no visible signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Overall, the galaxy's appearance suggests a well-established and relatively undisturbed system.
