The galaxy presents as a relatively smooth, lenticular or early-type spiral galaxy. The central bulge is prominent and appears mostly spheroidal in shape. A faint disk component is visible, though it lacks defined spiral arms. The galaxy exhibits a slight elongation, appearing somewhat cigar-shaped rather than perfectly circular. No major signs of tidal disturbances or ongoing mergers are apparent, although there is a slight asymmetry in the outer regions of the disk suggesting possible past interactions. The color profile indicates a predominantly older stellar population, with a noticeable lack of bright, young star clusters. There is a color gradient, transitioning from a redder central bulge to slightly bluer outer regions.
