The galaxy presents a disturbed morphology, with a shape that deviates significantly from a regular elliptical or spiral form. The primary structure appears elongated and somewhat cigar-shaped. There is evidence of ongoing or recent interaction, potentially involving a merger with another galaxy or significant tidal disturbances. A significant portion of light appears to be emitted from what looks to be an active star-forming region. It seems the overall color profile suggests a moderate redshift, with relatively bright emissions across the visible spectrum.
