The galaxy presents a predominantly smooth morphology, with a high degree of radial symmetry. It appears nearly elliptical in shape, with a moderate elongation along one axis, suggestive of a possible classification between elliptical and lenticular. The light distribution is concentrated towards the center, exhibiting a bright, unresolved core. There are subtle color gradients visible, with the central region displaying a somewhat yellowish-white hue, possibly indicative of an older stellar population. Fainter, bluer extensions can be observed away from the core in a somewhat disturbed halo. The lack of distinct spiral arms or dust lanes indicates that the galaxy is likely an early-type system, with a relatively quiescent star formation history. Weak asymmetric features suggest the possibility of minor tidal interaction or recent accretion event.
