The galaxy presents a generally elliptical morphology. A bright, concentrated nucleus dominates the central region, which could possibly indicate the presence of an active galactic nucleus. Diffuse light extends outwards from the core, displaying a slightly flattened disk-like structure. Subtle irregularities are noted along the outer edges. Patches of redder and possibly bluer areas are present within the galaxy's disk, and are suggestive of regions of star formation or dust obscuration. Overall, the object's structural features seem to be somewhat disturbed, potentially from a past or ongoing interaction.
