The galaxy presents a largely smooth, centrally concentrated light distribution with a color gradient trending from redder hues in the core to slightly bluer tinges in the outer regions. The elliptical morphology appears subtly elongated. There's a subtle indication of a disk-like structure. The galaxy does not appear to be undergoing any major merging activity or tidal disturbances. It displays an overall high concentration of light suggesting an older stellar population, though with signs of ongoing star formation.
