The galaxy appears as a centrally condensed object with a somewhat amorphous morphology. A bright, compact core dominates the galaxy's structure, exhibiting high luminosity. Diffuse, fainter emission surrounds the central region, extending in an irregular shape, and a slight asymmetry is visible, suggesting potential interactions or disturbances. There may be a hint of a very faint tidal tail or a very disturbed arm. Color gradients are subtle, transitioning from a bluer central core to a slightly redder halo, indicating possible variations in stellar populations or dust content. No distinct spiral arms or a clear disk structure are discernible. Overall, the galaxy presents a disturbed or irregular form, implying it is not a typical spiral or elliptical galaxy.
