The galaxy appears as an elongated, cigar-shaped structure with a relatively smooth overall morphology. It presents a concentration of light towards the central region, suggesting a prominent bulge. The color gradient transitions from a yellowish hue in the core to a slightly bluer tint in the outer regions, indicating potential variations in stellar populations and star formation activity across the galaxy. There's a faint suggestion of a disk-like structure, although the overall smoothness dominates. There is little evidence of significant disturbances or recent major mergers.
