The galaxy presents a largely smooth, elliptical morphology. There is a centrally concentrated bulge exhibiting a yellowish hue, indicative of an older stellar population. Moving outward from the core, the light gradually fades, and there is a faint, diffuse halo extending beyond the primary body of the galaxy. A slight discolouration towards red, compared to the central bulge, can be seen around the edges. There is no apparent spiral arm structure or dust lane obscuration visible within the resolution of this image. The galaxy does not show any obvious signs of major interactions or mergers.
