The galaxy presents a flattened, elliptical morphology. Its light profile appears smooth and centrally concentrated, suggesting a relatively old stellar population. There is a noticeable color gradient, with the central region exhibiting a slightly more yellow-red hue compared to the bluer outer edges. No distinct spiral arms or prominent dust lanes are visible. The overall shape is somewhere between round and cigar-shaped, with the galaxy appearing longer in one direction than the other, like an in-between elliptical galaxy. There are no obvious signs of major disturbances or mergers. The galaxy is a considerable distance away and appears to be a mature, relatively quiescent system with low-level star formation.
