The galaxy appears as an elongated, cigar-shaped structure. Its color profile exhibits a gradient, with a more intensely luminous, yellowish core transitioning to fainter, reddish-orange outer regions. The central bulge appears relatively smooth and featureless, suggesting a potentially older stellar population. The overall morphology indicates a disk-like galaxy seen edge-on, as there is minimal evidence of spiral arm structure. The smooth appearance suggests a higher probability of a smooth galaxy, though some minor disturbances cannot be ruled out. The lack of prominent dust lanes or distinct features hints towards a potentially lenticular or early-type spiral classification.