This galaxy exhibits a predominantly smooth morphology, with a nearly circular appearance. There is a slight elongation suggesting a possible deviation from a perfect sphere. The galaxy's color profile indicates a central concentration of older stellar populations, signified by a yellowish hue. Moving outwards, a faint blue tinge may suggest the presence of younger stars, though their overall contribution to the galaxy's light is minimal. Overall, the galaxy does not display prominent features such as spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions.
