The galaxy presents as a relatively smooth, centrally concentrated structure with an elliptical morphology. The core region exhibits a distinct yellowish-red hue, indicative of an older stellar population and/or dust obscuration. Moving outward from the core, the light transitions towards a bluer color, suggesting the presence of younger stars or differing stellar populations in the outer regions. The isophotes appear generally regular, though a slight deviation from perfect ellipticity might be present. There is no immediately discernible spiral arm structure or prominent dust lanes visible in this observation. The overall impression is that of a massive galaxy, potentially an elliptical or lenticular type.
