The galaxy presents a generally smooth and rounded morphology. There appears to be a concentration of light towards the center, suggesting a prominent galactic bulge. There is a slight color gradient observable, where the central region is more reddish, potentially indicative of an older stellar population, while the outer regions show a slightly more greenish/yellow hue. The galaxy exhibits a high degree of symmetry and lacks any obvious spiral arm structures or significant dust lanes. There appears to be no major disturbances or signs of an ongoing or recent merger event. The light distribution gradually decreases with distance from the center, lacking any sharp edges or abrupt changes in brightness.
