The galaxy presents a generally smooth, elliptical morphology. It appears highly concentrated with a bright, yellowish core that fades gradually into the surrounding halo. There is a slight elongation, but the overall shape is more akin to a slightly flattened spheroid rather than a strongly barred or spiral form. The overall color suggests an older stellar population and potentially a low rate of current star formation. No distinct features such as spiral arms or dust lanes are visible. There may be some very faint hints of a disk, but these are very subtle. The galaxy does not exhibit any obvious signs of ongoing major mergers or strong tidal disturbances.
