The galaxy appears as a moderately bright, elliptical-shaped object. Its light is concentrated towards the center, which exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. The outer regions of the galaxy display a gradual decrease in brightness, with a subtle color gradient towards reddish tones. The overall structure appears smooth, lacking prominent spiral arms or significant dust lanes. There is no apparent evidence of ongoing major mergers or strong tidal disturbances. Given its color and morphology, this galaxy likely contains a large population of evolved stars and a relatively low rate of current star formation.