The galaxy presents as a centrally concentrated, smooth system. It appears largely elliptical in shape, with a high degree of roundness. The light profile is dominated by a bright, yellowish core that gradually fades into a bluish halo. There is no visible dust lane or spiral arm structure. The color gradients suggest an older stellar population throughout much of the galaxy, with a possibility of some ongoing, low-level star formation hinted at by the bluer outer regions. There is no obvious evidence of tidal disturbances or ongoing mergers. The overall morphology suggests that this is likely an early-type galaxy.
