The object appears as a roughly elliptical galaxy, exhibiting a morphology with both smooth and featured components. The central region displays a bright, relatively smooth core that transitions into a more complex surrounding structure. Within this core, there is a slightly irregular and knotty formation, appearing brighter and possibly exhibiting ongoing star formation or active galactic nucleus activity.

The outer regions of the galaxy show evidence of some disturbance or tidal features. While not exhibiting a clear disk structure, there are hints of extended emission and asymmetries. This asymmetry could be due to minor gravitational interactions, possibly indicating a past or ongoing minor merger event. The general color profile indicates a mixture of stellar populations, with the bluer central core suggesting younger, hotter stars, and the overall green-tinged halo likely indicating a mix of older and younger stars, and possibly some dust extinction effects. The outskirts seem diffuse, hinting at a lower stellar density and possibly a halo of older stars or stripped material.
