The galaxy presents as a generally smooth, elliptical-like structure with an approximate redshift of 0.246. It exhibits a concentrated central region that radiates across multiple bands, appearing brightest in the redder bands with decreasing brightness toward the bluer bands. The galaxy shows no discernible spiral arm structure or prominent dust lanes. The overall shape deviates slightly from perfectly circular, showing some degree of elongation, and a slight cigar shape. There are hints of possible minor disturbances, though a major merger event is unlikely based on its morphology. The galaxy's color indices suggest a relatively evolved stellar population, consistent with a massive, early-type galaxy with a relatively low ongoing star formation rate.
