The galaxy appears to be a relatively smooth, elliptical type. It exhibits a high degree of radial symmetry, lacking any obvious spiral arm structures or prominent dust lanes. The light profile appears centrally concentrated with a gradual decrease in surface brightness with increasing radius. The central region is bright, with a yellowish hue, suggesting an older stellar population. The outer regions fade to a more reddish color, possibly indicating lower-level star formation or a dominance of older, cooler stars. There's no indication of major ongoing mergers or significant tidal disturbances in its morphology; it appears undisturbed. Overall, this galaxy presents the characteristics of an evolved system approaching quiescence, with minimal recent star formation activity.
