The galaxy presents as an elongated, disk-shaped structure with a relatively smooth overall appearance. The central region exhibits a brighter, more concentrated luminosity, suggesting a prominent bulge or nucleus. The color gradient transitions from a bluer hue in the central area to a slightly redder tone towards the outer edges, potentially indicating variations in stellar populations or dust content. There is evidence of a disk-like structure, but with no clearly defined spiral arms. The outer edges appear somewhat diffuse, with no major disturbances or signs of a major ongoing merger. Faint features suggest possible minor interactions or internal dynamic processes. The galaxy is moderately luminous, and has moderate mass, and low star formation rate.
