The galaxy presents as a flattened ellipsoid, appearing cigar-shaped with a notable central bulge. The light distribution is relatively smooth, indicating a dominant older stellar population. A faint disk is present, but less prominent than the bulge. There are no obvious signs of ongoing major mergers or significant tidal disturbances, and the structure appears largely undisturbed. Color gradients suggest the core is comprised of older stars than the galactic halo. The overall morphology appears to align with a galaxy that has largely ceased significant star formation, based on the low levels of blue light that can indicate ongoing or recent star formation.
