The galaxy presents as a spheroid with a smooth texture, possessing an elliptical-like morphology. The light profile is centrally concentrated, with an apparent decrease in surface brightness gradually diminishing outwards from the core. The core exhibits a yellowish-red hue, potentially indicative of an older stellar population. It appears that there is a bulge component that is more prominent on the left side, and on the right side there is a slightly smaller bulge. There is no clear evidence of spiral arms or significant dust lanes within the image. The overall structure suggests a galaxy that has undergone, or is undergoing a merger.
