The galaxy presents as a diffuse object of moderate angular size. A central, bright core is visible, suggesting a possible concentration of older stars or an active galactic nucleus. The outer regions exhibit an irregular morphology, with faint, extended arms or tidal features extending outwards from the main body of the galaxy. Patches of bluer light are scattered throughout the outer regions, indicating areas of ongoing star formation. There appears to be an interaction, possibly a merger, occurring as indicated by the irregular shape and faint arm-like structures.
