The galaxy presents as a flattened elliptical or lenticular type. A bright, concentrated central bulge dominates the morphology, exhibiting a yellowish-gold hue, which may indicate an older stellar population. The surrounding disk appears relatively smooth, with only subtle variations in brightness and color. The disk shows hints of bluer regions, suggesting the presence of some younger stars or ongoing star formation. The galaxy displays an overall elongated, cigar-like shape. There is no obvious indication of major mergers or significant tidal disturbances, although minor asymmetries could suggest past interactions.
