The galaxy presents as a single, relatively smooth object. It displays a roughly elliptical morphology, with a centrally concentrated bulge region that diffuses outward into a less defined disk. The central bulge exhibits a brighter, more uniform luminance, suggesting a higher stellar density. The outer regions of the galaxy appear bluer in hue compared to the central areas. There are no apparent spiral arm structures or significant dust lane features visible in this image. Faint irregularities in the outer regions might suggest minor disturbances or interactions, but the dominant impression is of a relatively undisturbed system. The overall color profile indicates ongoing but not excessively high star formation activity.
