The galaxy presents as a somewhat elliptical, though not perfectly spherical, luminous structure. Its core region exhibits a bright, concentrated glow, suggesting a high density of stars or possibly an active galactic nucleus. The light from the central region is yellowish-white, which could indicate a population of older stars. Fainter and somewhat diffused light extends outwards from the core, which exhibits a hint of spiral structure in a very diffuse disk. There appears to be a minor disturbance of the galaxy's morphology, possibly due to interactions with a smaller companion or an ongoing merger event. The edges of the galaxy are indistinct, fading into the background, and it's difficult to discern any distinct spiral arm structure or dust lanes. There is a very faint bluish color in some of the outermost edges of the galaxy, which may indicate some ongoing star formation.
