The galaxy appears as a centrally concentrated, smooth object with a somewhat elliptical morphology. The central region exhibits a brighter, yellowish-white hue, suggesting a population of older stars. Surrounding this core, a less defined, bluer halo extends outwards. This halo likely contains a population of younger, hotter stars and regions of ongoing star formation. There is faint evidence of a disk or spiral structure embedded within the halo, but no distinct arms are readily apparent. Overall, the galaxy does not display any obvious signs of major disturbances or ongoing mergers.
