The galaxy presents a generally smooth, elliptical morphology. The core exhibits a high degree of central concentration, displaying a bright, yellowish hue indicative of an older stellar population. The galaxy appears largely undisturbed, showing no significant signs of ongoing mergers or major tidal interactions. There are no apparent spiral arms or a distinct disk structure. The light distribution suggests a relatively homogenous stellar population throughout the galaxy, with the central region being more luminous. 
