This galaxy appears to be a relatively smooth, centrally concentrated object. The overall morphology is largely spheroidal, indicating it may be an elliptical galaxy or a lenticular galaxy seen at a shallow inclination angle. There is a concentration of light with a yellow hue, implying a population of older stars. A small, redder region is visible near the central bulge, which could indicate an area of more recent, lower-level star formation or perhaps a heavily dust-reddened population. The galaxy doesn't present significant signs of major ongoing mergers or tidal disturbances, although a minor perturbation cannot be ruled out based on the image data alone. It exhibits a modest degree of star formation.
