The galaxy presents a somewhat elliptical morphology, though some degree of disturbance is apparent. The color profile suggests a predominantly older stellar population, with a noticeable concentration of light towards the central region indicative of a bulge. There are some faint blue-ish wisps visible in the outer disk which may be signs of some ongoing low-level star formation. The overall smoothness of the galaxy indicates a relatively evolved system, although subtle irregularities suggest potential past minor interactions or internal dynamical processes. Based on this evidence, this galaxy would likely be categorized as an intermediate stage system nearing the quiescent state, likely an early-type spiral or lenticular galaxy.
