The galaxy presents a generally smooth and elliptical morphology. There is a central bulge that is visible, with a diffuse halo extending outwards. The galaxy exhibits a slight elongation but appears mostly round. There is minimal evidence of spiral arms or significant dust lanes. Its color is primarily bluish-white, suggesting some presence of younger stellar populations, though the smoothness implies that star formation is likely not exceptionally vigorous. There are indications of potential minor disturbances in the outer regions, hinting at possible past or ongoing interactions. Overall, the galaxy appears to be an intermediate type, transitioning between a pure elliptical and a spiral, possibly an early-type spiral or a lenticular galaxy.
