The galaxy appears to be a relatively smooth, elliptical system. It displays a centrally concentrated bulge that transitions smoothly into a fainter, more diffuse halo. There is some suggestion of a slight elongation or a weak disk-like component, but overall the structure is dominated by a spheroidal shape. The galaxy exhibits a color gradient, with a bluer hue in the outer regions suggesting the presence of younger stellar populations and ongoing star formation. There are no apparent spiral arm structures or prominent dust lanes. The overall morphology suggests a mature galaxy with a significant fraction of old stars, but with some residual star formation activity in the outer regions.
