The galaxy presents as a centrally concentrated, fairly smooth object with a noticeable elliptical morphology. The core region exhibits a bright, yellow-orange hue, suggesting a significant population of older stars. There is a subtle color gradient, transitioning to a bluer, fainter periphery. No distinct spiral arm structures or dust lanes are readily apparent. The overall appearance indicates a high probability of the galaxy being an early-type galaxy, specifically elliptical or lenticular in nature, with little current star formation activity. The lack of visible disturbances suggests a gravitationally relaxed system, likely not undergoing any major merging events.
