The galaxy presents as a generally smooth and rounded structure. Its morphology appears primarily spheroidal. The central region exhibits a bright, concentrated luminosity, suggestive of a significant stellar density or potentially an active galactic nucleus. The overall color is yellowish-orange, indicating a population of older stars with lower rates of on-going star formation and dust obscuration. There is very little indication of spiral arm structures or significant star formation regions. The galaxy appears undisturbed, without significant signs of tidal interactions or ongoing mergers. A very faint and diffuse halo extends beyond the bright central region.
