The observed galaxy presents as a somewhat disturbed, disk-like structure. There appears to be a central, bright region with a concentration of light that may indicate a bulge. Extending from this core, a flattened structure exhibits a non-uniform distribution of light. One arm-like feature may be present on the outer regions. Overall the galaxy does not appear to be of completely regular morphology. Evidence indicates a possible ongoing or recent interaction, marked by asymmetries. The galaxy presents a distinct blue tinge.
