The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. There appears to be a lack of distinct spiral arms or a prominent disk structure. The galaxy is generally round in appearance. The light distribution suggests a relatively uniform stellar population, with no clear signs of active star formation regions or dust lanes visible in this image. There are no immediately obvious signs of a major ongoing merger or significant tidal disturbances, although subtle irregularities in the outer isophotes cannot be ruled out without deeper observations. The galaxy exhibits a redder hue in the central regions. Overall, the galaxy appears to be a relatively undisturbed, passively evolving system.
