The galaxy presents an elongated, somewhat irregular morphology. It displays a generally bluish hue across its structure. There is evidence of potential disturbances in its form, possibly indicating minor interactions or ongoing merger activity. The light is not evenly distributed throughout, with some regions appearing brighter than others. The overall impression is of a galaxy that is not fully relaxed in its morphology, suggesting either recent interactions or ongoing internal processes that are shaping its structure. There is potentially a disk structure present, but this is difficult to ascertain due to the disturbances.
