The galaxy appears to be elliptical in shape, though not perfectly spherical. The light distribution suggests a relatively smooth structure, indicative of an older stellar population, with a concentrated central region that graduates outwards. There is a subtle elongation; this may hint at an ongoing minor interaction, though the overall morphology suggests it is largely undisturbed. Color appears slightly green, which could indicate a larger amount of heavy elements. The edge is fairly sharp, which could indicate that star formation ceased long ago.
