The galaxy presents as a relatively compact, smooth structure with a dominant central bulge. The overall shape is elliptical, verging on spheroidal, with no clear spiral arm structure visible. The light distribution is concentrated towards the center, suggesting a high degree of stellar density in the core. The color appears to be yellowish-orange, indicating a population of older, cooler stars. There is minimal evidence of recent star formation activity. The overall morphology suggests an early-type galaxy that is in a relatively evolved state. No signs of ongoing mergers or major disturbances are apparent.
