The galaxy presents a largely smooth, elliptical morphology. It appears nearly round in shape, exhibiting little to no discernible disk structure or spiral arms. A bright, concentrated central bulge dominates the galaxy's luminosity profile. The galaxy exhibits a relatively smooth gradient in color, shifting subtly from a slightly bluer hue at its core to a marginally redder tone in its outer regions. There is no indication of major disturbances or ongoing merger activity within the visible structure of the galaxy, though minor interactions cannot be entirely ruled out. The galaxy's apparent size is relatively small, suggesting it is either intrinsically compact or located at a considerable distance. The estimated color indices suggest a population of older stars, though some ongoing star formation cannot be excluded based on the slight blueing towards the central region.
