This galaxy exhibits a relatively smooth morphology, appearing largely featureless upon visual inspection. It appears to be primarily elliptical or lenticular in shape, with a significant bulge component. The galaxy has a central, bright, and compact core, suggesting a high concentration of stars in that region. There is some indication of a slight disk or extension in the galaxy's structure, but it's not heavily defined. Color gradients suggest an older stellar population; light from the galaxy is more red, indicating an evolved stellar population. Indications of current star formation are low. There are no signs of major interactions or mergers. The round shape indicates that it is not rotating rapidly. The galaxy is a generally undisturbed system.
