The galaxy presents as an elliptical or lenticular type, with a generally smooth light distribution. The central region exhibits a concentrated core, which suggests a higher density of stars. The galaxy's light profile appears somewhat rounded. There are some signs of minor disturbances in the outer regions, but overall the galaxy appears fairly settled. Color gradients suggest a population of older stars dominating the central regions, while bluer hues may indicate younger stars and star formation activity in the surrounding regions. The galaxy is relatively compact and of intermediate mass. The star formation rate is relatively low.
