The galaxy presents a predominantly smooth, centrally concentrated morphology, appearing elliptical in shape. There is some evidence of low-level disturbance or features deviating from a purely smooth profile. The central region exhibits a bright, concentrated core, suggesting a high density of stars or a possible active galactic nucleus. The color gradient indicates a blue core and red periphery. There are no discernible spiral arms or bar structures. The faint, extended halo suggests possible tidal interactions or previous minor mergers.
