The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light profile suggests a centrally concentrated bulge, exhibiting a yellowish-white hue. Fainter, bluer regions are observed extending from the central bulge, suggestive of a disk. The disk appears relatively smooth, with little indication of prominent spiral arm structure or significant dust lanes at this resolution. Overall, the galaxy displays characteristics of an early-type spiral, potentially an S0, viewed edge-on. A lack of obvious distortions suggests it is relatively undisturbed by recent major mergers, but there may be some minor disturbance apparent.
