The galaxy presents an elliptical morphology with a relatively smooth light distribution. It exhibits a central, bright core that gradually fades into the outer regions. The overall color appears to be yellowish-white, indicative of an older stellar population. A subtle blueish hue is detectable in some of the outer regions of the galaxy, potentially suggesting areas of ongoing, or recent, star formation. No spiral arms or significant dust lanes are obviously apparent. The galaxy does not appear to be undergoing a major merger, although subtle irregularities in its shape suggest the possibility of minor gravitational interactions or disturbances. The shape deviates slightly from being perfectly circular, appearing somewhat elongated.
