The galaxy presents as a luminous, elliptical-shaped object with a relatively smooth overall appearance. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The light is strongly concentrated, fading gradually towards the outer edges. The galaxy's color appears to be yellowish-orange, indicative of an older stellar population and reduced recent star formation. There are no obvious spiral arm structures or dust lanes visible within the image. Based on the morphological classification, the galaxy exhibits a smooth, round profile, with some slight disturbances apparent. No signs of ongoing merger activity are clearly visible, though some minor disturbances may be present in the outer regions of the galaxy.
