The galaxy presents an elliptical morphology, appearing mostly smooth in structure. There is a suggestion of an ongoing merger event, possibly involving a smaller companion. The galaxy displays a radial color gradient, with a bluish core and a yellowish-orange halo. This may reflect a central concentration of younger, hotter stars, or a potential active galactic nucleus. Star formation rate appears to be low, but not totally absent. The overall shape is somewhat irregular, deviating from a perfectly elliptical profile, which may be further evidence of tidal interactions.
