The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness towards its outer edges. There is an absence of distinct spiral arm structures or prominent dust lanes within the visible spectrum. The galaxy appears somewhat rounded in shape, deviating slightly from a perfect circle. Its overall color suggests a relatively older stellar population with a low rate of ongoing star formation. There are no obvious signs of major tidal disturbances or ongoing merger events. Minor disturbances are possible but not clearly apparent within the image resolution. The galaxy demonstrates a moderate redshift, indicating its location at a considerable cosmological distance.
