The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated luminosity profile. The central region is significantly brighter, with a gradual decrease in luminosity towards the outer edges. Its shape is generally round with an ellipticity that suggests a slightly flattened structure. There is little indication of spiral arms or significant dust lanes. The color profile is dominated by yellowish hues in the central region, indicating an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of younger stars or some ongoing, but minimal, star formation. There is a subtle asymmetry in the color distribution, suggesting potential minor disturbances or interactions.
