This galaxy presents as a relatively smooth, elliptical structure. It exhibits a somewhat elongated shape but lacks any visually distinct spiral arm features or a prominent central bar. The color gradient transitions from a more yellowish-orange core to a slightly bluer halo, suggesting a potential aging stellar population concentrated in the center with possibly younger stars distributed in the outer regions. Faint irregularities in the outer halo might indicate minor tidal interactions or past mergers, although the overall morphology suggests it is not undergoing a major disruptive event. There appears to be low levels of on-going star formation.
