The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The central region displays a yellowish-white hue, suggesting a population of older stars. Fainter, bluer light surrounds the central region, potentially indicative of younger stars and ongoing star formation within a disk-like component. The overall appearance is relatively smooth, with no obvious spiral arm structures or significant dust lanes visible in this imagery. There may be some minor disturbances in the outer regions, although it mainly appears as a single object with an absence of major merging features.
