The galaxy presents a roughly elliptical morphology, appearing somewhat flattened. Its color profile is complex, displaying a central region with a distinct blue hue, suggesting the presence of younger, hotter stellar populations. The outer regions exhibit a more yellow-red coloration, possibly indicating older, cooler stars, or dust obscuration. There is evidence of some disturbance in the morphology, it could be in the early phases of a minor merger event or exhibiting internal asymmetry. There is likely no significant ongoing star formation within the galaxy's core, and a very low rate galaxy-wide, given the redness. It seems to lie somewhere between being a spiral and elliptical galaxy. 
