The galaxy presents as a flattened, elongated structure, suggestive of an edge-on or highly inclined disk galaxy. The central bulge exhibits a bright, yellowish hue, indicating a significant population of older stars. The disk component shows a bluer color gradient extending outward from the bulge, implying the presence of younger, star-forming regions. The overall morphology appears smooth, with no obvious signs of strong spiral arm structure or major disturbances. There is a slight asymmetry visible in the outer regions of the disk, hinting at possible minor interactions or internal asymmetries within the galactic structure. The shape is cigar-like, significantly longer than wide. There is little evidence of recent merger activity.
