The galaxy presents as a largely featureless, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominating this region. The radial light profile descends smoothly from the core, showing a gradual transition into a more diffuse outer halo. The overall color of the galaxy appears to be red-shifted. A small irregular feature of bluish light is present on one side. This could potentially be a region of on-going star formation or possibly a smaller object experiencing a minor merger with the primary galaxy. The lack of defined spiral arms or dust lanes further supports a classification as an early-type, potentially lenticular, system. Its roundness suggests that we are observing it close to face-on.
