The galaxy presents as a highly elongated, cigar-shaped structure. Its light profile is generally smooth, with a concentrated central region that gradually fades towards the edges. There is little evidence of spiral arms or distinct substructures, suggesting a relatively featureless morphology. Color gradients across the galaxy are subtle, displaying a slightly bluer hue in the central region, transitioning to redder tones at the outskirts, possibly indicating variations in stellar populations or dust content. The galaxy appears undisturbed, with no obvious signs of ongoing mergers or major tidal interactions.
