The galaxy presents as a single, relatively smooth structure with a centrally concentrated bulge. The overall morphology appears elliptical or lenticular due to the lack of discernible spiral arms. The galaxy exhibits a color gradient, with the core appearing more yellow-orange, possibly indicating an older stellar population. The outer regions show hints of a bluer hue, but the contrast is minimal. There is a slight elongation, but the shape is generally round. There is evidence of a tidal feature or minor disturbance extending from the main body of the galaxy. There is a strong indication that the galaxy is quite massive, and the data suggests there is minimal current star formation occurring. There is a possibility of the galaxy being in an ongoing or recent merger event based on the overall appearance.
