The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a prominent central bulge that is brighter and more concentrated than the surrounding galactic disk. The light distribution suggests an older stellar population, particularly within the bulge region. There is a slight elongation to the galaxy's shape, appearing somewhat cigar-shaped. No distinct spiral arms are visible. Minimal dust lanes or star-forming regions can be discerned. The galaxy does not appear to be undergoing any major merger events, although there may be signs of minor disturbances in its structure. Overall, it appears to be a relatively quiescent galaxy with a dominant spheroidal component.
