The galaxy appears to be a relatively smooth, elliptical-type galaxy with an approximate diameter of 6 kiloparsecs. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness towards the outer regions. The core region displays a yellowish hue, suggesting an older stellar population. There is minimal evidence of spiral arm structure or significant dust lanes. The morphology appears undisturbed, with no obvious signs of major mergers or tidal interactions. There is a faint blue-ish halo surrounding the main body, possibly indicating a region of recent star formation, or a population of younger stars. Overall, the galaxy presents a relatively quiescent and evolved appearance.
