The galaxy presents a generally smooth and rounded morphology. There is a bright, concentrated central region, likely indicating a significant bulge component. The outer regions exhibit a gradual decrease in luminosity, lacking sharp or well-defined spiral arm structures. The overall color appears relatively uniform, with subtle variations suggesting a mix of stellar populations, and potentially active star formation regions. Faint extensions hint at possible tidal interactions or minor disturbances. The galaxy is not perfectly spherical, but rather exhibits a slight flattening, possibly indicative of a disk component, although it is not clearly resolved in the image.
