The galaxy presents a generally smooth and elliptical morphology. A significant fraction of the galaxy's light is concentrated in its central region, suggesting a prominent bulge. The galaxy appears largely spheroidal, with only a slight deviation towards a more elongated shape. There is no clear evidence of a distinct disk component. The colour profile suggests the presence of both older stellar populations, indicated by reddish hues, and regions with ongoing or recent star formation, suggested by the subtle presence of bluer colours. The galaxy is not currently undergoing any major mergers, though minor disturbances are possibly indicated by slight asymmetries.