The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy seen nearly edge-on. A bright, centrally concentrated bulge is observed, which appears relatively smooth in texture. The disk component exhibits a subtle color gradient, trending from bluer hues toward the edges, potentially indicating regions of recent or ongoing star formation, to redder hues toward the center. The morphological classification aligns with a cigar-shaped galaxy, showing no signs of major mergers or disturbances. The galaxy possesses moderate mass and is undergoing low levels of star formation.
