The galaxy exhibits a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is centrally concentrated, with a gradual decrease in brightness moving outwards from the core. The galaxy possesses a moderate degree of roundness in its overall shape. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity, although a subtle asymmetry in the outer regions might indicate a past minor interaction. The color suggests an older stellar population, with a relatively low rate of star formation within the galaxy. 
