The galaxy presents a largely smooth and centrally concentrated morphology. It appears elliptical in shape, showing a gradual decline in brightness from the core outwards, with no distinct spiral arms or bar-like features visible. The color profile indicates a likely evolved stellar population, with a yellowish-orange hue dominant in the central region, potentially indicative of older, cooler stars. There is no obvious dust lane obscuring the galaxy's light. No signs of strong tidal interactions or major merger events are readily apparent, although a faint asymmetry might suggest a minor disturbance. Based on the light profile, it is a galaxy that might be a quiescent or low star-forming system.