The galaxy exhibits a roughly elliptical morphology with a notable central bulge. The core region displays a concentrated luminosity, appearing yellowish-white in color, indicative of a population of older stars. Moving outward from the core, the color transitions towards a bluer hue, suggesting the presence of a younger stellar population or regions of active star formation within the galaxy's disk. There appears to be little in the way of spiral arm structure, with light being diffusely distributed. The outer regions of the galaxy fade gradually into the background sky, with no signs of significant tidal features or major disturbances, pointing to a relatively undisturbed evolutionary history.
