The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, concentrated light profile. The central region appears bright and diffuse, with a gradual decrease in luminosity toward the outer edges. The overall color index indicates a population of older stars. There is no apparent spiral structure, bar feature, or significant dust lane visible in the image. Subtle disturbances or asymmetries are observed suggesting minor gravitational interactions, but is not the dominant feature. The galaxy has an intermediate mass range and a modest star formation rate.
