The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge, with a luminosity that decreases gradually outward. The color profile is relatively uniform, displaying a redder hue overall, which is indicative of an older stellar population. There are no prominent spiral arms or dust lanes visible, supporting its classification as an early-type galaxy. There is a faint, diffuse halo surrounding the central region. It is difficult to discern any fine details due to the distance and resolution of the image. There are no signs of any major disturbances or tidal features, suggesting that the galaxy is not currently undergoing a significant merger event.
