The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity with a yellow-white coloration, suggesting a significant population of older stars. Moving outward from the core, the light gradually diffuses. The lack of defined spiral arms or prominent dust lanes indicates that the galaxy is likely an early-type galaxy, potentially an elliptical or lenticular galaxy. There are no obvious signs of ongoing major merger activity, though there are hints of possible minor disturbances in the outer regions. The overall structure appears to be largely undisturbed, with a high degree of rotational symmetry and a relatively round shape.
