The galaxy presents as a roughly elliptical morphology, appearing flattened along one axis. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. Moving outwards from the core, the luminosity gradually decreases, transitioning into a more diffuse halo. The overall color profile indicates a population of older stars, as evidenced by the reddish hue of the central bulge, with a hint of younger, bluer stars residing primarily in what appears to be a faint disk structure. There are some subtle signs of possible tidal disturbances.
