The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated, bright, yellowish-white glow, suggesting a dense population of older stars. Moving outward from the center, the light gradually diminishes, and there's a subtle shift toward redder hues, indicating an aging stellar population in the outer regions as well. No distinct spiral arms or prominent dust lanes are visible. The galaxy shows a high degree of circularity. No signs of major ongoing merger activity or significant tidal disturbances are readily apparent. Overall, it appears to be a quiescent galaxy, likely an elliptical or lenticular type.