The galaxy presents as a somewhat elliptical, lenticular structure with a prominent central bulge exhibiting a yellowish hue. The surrounding disk appears less defined, with faint hints of bluish regions, potentially indicative of younger stellar populations or ongoing star formation. The overall morphology suggests a system that is likely undergoing a transition from a spiral-dominated structure to a more quiescent state. The color distribution points toward an older stellar population dominating the central region, with younger stars concentrated, if sparsely, in the outer regions of the disk. There is no apparent strong tidal disturbance or close companion galaxy to suggest a recent major merger event, although subtle asymmetries or faint disturbances could be present within the system. The galaxy is relatively smooth in appearance, lacking distinct spiral arms or significant dust lanes.
