The galaxy presents an elliptical morphology with a high degree of central concentration. The core is bright and relatively smooth, with a gradual decrease in luminosity towards the outer regions. The color profile appears generally uniform across the galaxy, lacking prominent features of recent star formation. There is a slight elongation to the galactic disk, which suggests there might be a moderate degree of rotation or tidal influence. Overall, the galaxy appears to be a relatively quiescent system, likely dominated by an older stellar population.
