The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright core region, likely indicative of a significant stellar population or perhaps an active galactic nucleus, though further spectral analysis would be needed to confirm the latter. The galaxy appears largely undisturbed, with no obvious signs of tidal features or ongoing major mergers. There is a slight elongation to the galactic structure, but overall it is relatively round. Color gradients suggest a possible change in stellar population from the core to the outer regions, with a bluer hue apparent in the periphery, indicating possible recent star formation compared to the core. The overall red color suggests this is a relatively massive, evolved galaxy.
