This galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, suggesting a concentration of older stellar populations or potentially an active galactic nucleus, although further spectral analysis would be required to confirm the presence of an AGN. There is a subtle flattening of the galaxy's shape with a slight elongation, and a small hint of possible disk-like morphology, though this is not pronounced. The outer regions fade smoothly, indicating a lack of significant star formation in the outskirts, and a population of older, redder stars. There is no obvious evidence of spiral arms, rings, or strong tidal disturbances, which suggests that the galaxy is relatively undisturbed. The overall color is moderately red. The galaxy displays a smooth, largely featureless profile, with only a minor irregularity present.
