The galaxy presents a predominantly smooth, elliptical morphology with high degree of central concentration. The luminous core is surrounded by a more diffuse halo of light, suggesting a relatively old stellar population and minimal ongoing star formation. The galaxy exhibits a largely undisturbed structure, with little evidence of tidal features or recent merger activity. A slight color gradient is visible, with the central region appearing yellower and the outer regions somewhat bluer. This subtle bluing in the outer regions may indicate a small amount of younger stars in the outer regions. The galaxy is well-resolved, but lacks any distinct spiral arms or prominent dust lanes, indicative of an early-type galaxy.
