The galaxy appears to be a relatively smooth, elliptical type, exhibiting a concentrated central bulge. Its color index suggests a population of older stars, with a yellowish-red hue dominating the overall appearance. The galaxy's shape is not perfectly spherical, showing a slight elongation or cigar shape. There is no obvious evidence of spiral arms or significant dust lanes, although a slight feature or disk could be present in the galaxy, which would indicate the potential for ongoing minor star formation, but the lack of a prominent blue colour indicates this is unlikely. There also seems to be no sign of major disturbances or interactions with other galaxies, suggesting a relatively isolated existence. The overall structure indicates a galaxy that has likely undergone significant evolution, with the majority of its star formation having occurred in the past.
