The galaxy presents as a centrally concentrated object, with a largely smooth morphology. The overall color index suggests a system dominated by older stellar populations, with a possible moderate star formation rate. There's a noticeable lack of defined spiral arms or a distinct disk structure. The object exhibits a predominantly elliptical shape, tending toward roundness. No significant signs of ongoing mergers or major disturbances are apparent, although minor interactions cannot be ruled out. The central bulge region appears quite prominent and bright. The galaxy is relatively compact.
