The galaxy presents an elongated, elliptical morphology. The core is a bright, concentrated region with a yellowish hue, suggesting an older stellar population. Proceeding outward, the galaxy appears relatively smooth, with a diffuse halo extending further than the central region. This halo seems to be bluer in some areas, suggesting the presence of some younger stars mixed in with the older population. 

Overall, the galaxy exhibits characteristics consistent with an early-type, possibly lenticular, galaxy with a considerable spheroidal component. There is some suggestion of a disk-like structure, but it is not prominent and is seen nearly edge-on. Faint features suggest slight disturbances within the galaxy, but there are no major mergers indicated. The relatively smooth appearance and color gradients imply a degree of evolved stellar populations.