The galaxy presents as a slightly elongated, disk-like structure with a concentrated central bulge. The overall color is yellowish-orange, suggesting a population of older stars with a possible lower rate of current star formation. There is a hint of bluer color on the edges, perhaps indicating the presence of younger stars in the disk. The galaxy appears relatively smooth in texture, with no readily apparent spiral arm structure or significant dust lanes. It seems undisturbed, exhibiting no strong signs of tidal interactions or ongoing mergers. The galaxy's profile is moderately flattened, neither perfectly round nor highly elongated.
