The galaxy appears to be a relatively smooth, elliptical system. Its core exhibits a bright, concentrated luminosity, potentially indicating an active galactic nucleus or a dense stellar population. The galaxy's light profile is characterized by a centrally concentrated bulge that fades into a more diffuse halo. There is a slight asymmetry and some suggestion of possible tidal interaction, but the overall structure seems largely undisturbed. The colour is bluer closer to the core of the galaxy, indicating some ongoing star formation, or a relatively young stellar population. The galaxy does not show a distinct disk structure.
