The galaxy presents a generally elliptical morphology, with a notable central bulge that appears bright and concentrated. The overall color gradient suggests a slightly redder hue in the central region. Fainter extensions or a disk-like structure seem to be present around the central bulge. There is evidence of possible tidal features or minor disturbances on the outer edges, hinting at past gravitational interactions. A small percentage of the galaxy shows signs of merging or disrupted morphology, with some areas appearing irregular and diffuse. 
