The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroidal in form. There is a noticeable color gradient, with a yellowish-white core, transitioning to a bluish halo in the outskirts. The lack of defined spiral arms or a prominent disk structure supports the smooth morphology. There is some minor asymmetry within the main body of the galaxy, with a slight extension of the blue halo on one side, possibly indicative of tidal interactions or recent minor merger events. The central region exhibits a high degree of light concentration, which may point to an aging stellar population and a prominent bulge. Overall, the galaxy is relatively isolated, showing little evidence of major ongoing interactions or disturbances despite the slight asymmetry in the halo. The galaxy appears relatively compact.
