The galaxy presents as an elongated, somewhat cigar-shaped structure. Its central region appears bright and diffuse, exhibiting a yellowish-orange hue, possibly indicating an older stellar population or significant dust obscuration. Moving outwards from the core, a subtle disk-like structure emerges, showing a bluer tinge, suggesting the presence of younger, hotter stars and active star formation. There's a hint of irregularity in the galaxy's overall form, potentially indicative of an ongoing or recent interaction, with subtle disturbances in the outer disk. There is a strong indication of a merger, and the galaxy seems to have some ongoing star formation.
