The galaxy presents as a singular, centralized object. Its light profile appears relatively smooth, with no apparent spiral arm structure or distinct bar. The morphology seems to be primarily spheroidal in nature. The galaxy exhibits a yellowish-white color, indicative of a stellar population that is potentially older and less actively forming stars compared to bluer galaxies. There is no significant sign of tidal disturbances or ongoing major merger events based on the images; its structure appears largely undisturbed. The overall impression is that this galaxy is likely an elliptical or possibly an early-type spiral with a dominant bulge. The relative uniformity of color and the lack of distinct features points toward a more evolved stellar population.
