The galaxy presents an elliptical morphology, exhibiting a smooth, centralized luminosity profile characteristic of early-type systems. The light distribution is concentrated towards the core, with a gradual decrease in surface brightness outwards. The major to minor axis ratio suggests a moderate ellipticity, appearing somewhat flattened. A slight inclination is observed. A subtle color gradient is noticeable, with the central region displaying a slightly yellower hue compared to the outer regions, implying a potential difference in stellar populations or dust content. No distinct features, such as spiral arms or prominent dust lanes, are apparent within the observable structure.
