The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge that graduates outward in luminosity. The primary color gradient shifts from a yellow-white hue in the center to a slightly bluer tinge in the outer regions of the disk. There is a suggestion of a disk-like morphology, though it appears relatively smooth with limited discernible spiral arm structure. The observed morphology is consistent with a relatively evolved system. There are some subtle irregularities in the outer edges of the galaxy, suggesting possible minor tidal disturbances or interactions. The overall appearance indicates a system with suppressed star formation compared to its mass.
