The galaxy presents as a somewhat elongated, elliptical-like structure. Its light profile appears smooth, with a concentrated, bright central bulge that fades gradually outwards. There are hints of a flattened disk component, though not sharply defined. The color is predominantly yellowish-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. The elongation suggests it is not perfectly spherical but is rather seen at an angle. There do not appear to be any prominent spiral arms, or any major signs of recent tidal disturbances or mergers.
