The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a high degree of concentration and appears a yellow-orange hue. This suggests an older stellar population dominating the galactic center. Moving outward from the core, the galaxy maintains a generally smooth texture with a gradual decrease in luminosity. There is no evidence of distinct spiral arms or significant dust lanes. The overall morphology appears largely undisturbed, showing no strong signs of ongoing major merger events. The galaxy appears to be relatively round, with the ratio of the major to minor axes being close to unity. A slight disturbance may be present, but it's very minimal.
