The galaxy exhibits a generally elliptical morphology, appearing largely spheroidal and smooth. The core region displays high luminosity, with a concentrated bright central bulge. There is a slight elongation observable, suggesting a deviation from perfect circularity, though it leans towards roundness. Emanating from the central region, a subtle disc-like structure may be present, though it is not distinctly defined. Additionally, there appears to be some disturbance in the outskirts of the object, possibly suggesting a minor interaction or tidal features. Patches of redder emissions are apparent, these are likely to be areas with older stellar populations or higher dust density. Overall, the galaxy appears to be an early-type galaxy, likely an elliptical or lenticular galaxy, possibly undergoing some form of interaction or disturbance.
