The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. There is a slight elongation, suggesting a transition towards a more lenticular, or possibly even a spiral form.

The central region displays a concentrated brightness, indicating a likely bulge component with a population of older stars. The outer regions appear less luminous, with a gradual decrease in light intensity. This suggests a diminishing stellar density further from the galactic center.

There may be subtle, faint features indicative of a disk, but the overall smoothness and lack of distinct spiral arms imply that the galaxy is dominated by its spheroidal component. The color profile indicates a yellow to orange hue in the central region, which transitions to a bluer tint in the outer regions. This may represent a younger stellar population present in the arms of the galaxy.
