The galaxy presents as a fairly smooth, centrally concentrated object with a generally elliptical morphology. The central region exhibits a yellowish hue, suggesting a population of older, redder stars. Moving outward from the core, the color transitions to a bluer, fainter halo. There is no strong evidence of spiral arm structure or significant dust lanes. A slight asymmetry is visible in the outer regions, suggesting a potential minor disturbance or interaction with a smaller companion, although this is not definitive from the image. The overall smoothness and color gradients suggest a relatively evolved system with ongoing, but potentially declining, star formation.
