This galaxy presents a predominantly smooth morphology. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The overall shape approximates a slightly flattened spheroid. The light distribution appears relatively uniform, with a gradual decline in intensity moving outward from the center. There is a subtle suggestion of a disk component, but the light is mostly concentrated towards the center. No distinct spiral arms or significant dust lanes are discernible within the resolution of the image. Minor irregularities in the outer edges may indicate a past interaction or disturbance, but there is no strong evidence of any major merging activity, though a slightly disturbed appearance is noticeable.
