The galaxy presents a primarily smooth morphology, indicative of an elliptical or lenticular type. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density and potentially the presence of an active galactic nucleus, though further spectral analysis would be necessary to confirm this. The galaxy displays a slight elongation, deviating from a perfectly spherical shape and is relatively undisturbed, with only minor visual asymmetries or tidal features noticeable. The color profile of the galaxy appears to be relatively uniform across the structure, with subtle color gradients towards the outer edges. A possible faint disk structure can be hypothesized. Overall, the galaxy seems to be a massive, evolved system with modest star formation, primarily composed of older stellar populations.
