The galaxy appears to be relatively compact, exhibiting a somewhat amorphous structure rather than a well-defined spiral or elliptical shape. A bright, concentrated central bulge is evident, suggesting a high stellar density in the galactic core. Surrounding the central bulge, a fainter, diffuse disk component is present, displaying a slightly irregular morphology. Hints of possible tidal features or minor disturbances are observable on the periphery of the galaxy, implying potential gravitational interactions with other galaxies or past merger events. Overall, the galaxy presents a non-smooth and somewhat disturbed appearance, warranting further investigation into its evolutionary history and potential interactions within its environment. The color distribution indicates a possible mix of stellar populations, with bluer regions possibly indicating younger stars or active star formation.
