This galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, diffuse light distribution overall, with a concentration of light towards the central region. The core appears yellowish, possibly indicating an older stellar population. Moving outwards from the core, we see a transition to a bluer hue, suggestive of younger stars or ongoing star formation activity within a disk-like structure. There may be a sign of a minor interaction or disturbance with a smaller neighboring galaxy or the remnant of a past merger event.
