The galaxy presents as a generally smooth, elliptical form. It exhibits a centrally concentrated bulge, with a radial decrease in luminosity moving outward from the core. The galaxy appears largely homogenous in color, trending toward redder hues, particularly in the central region. The outer edges of the galaxy show a slight bluer tint, indicative of younger stellar populations, though to a small degree. There is a subtle hint of asymmetry in the extended halo, possibly suggesting a minor interaction or past merger event. Overall, the light is consistent with an evolved stellar population with relatively low ongoing star formation. No distinct spiral arms or prominent dust lanes are visible.
