The galaxy presents as a centrally concentrated structure with an elliptical morphology. It exhibits a smooth light distribution, appearing relatively featureless upon visual inspection. There's some visual evidence of possible disturbance.

Based on observed colors, this galaxy appears to host a population of older stars and is considered to be a relatively massive galaxy. Its spectral properties indicate ongoing star formation, though not at a particularly high rate, indicating that it might be in a transition phase. The image suggests that the galaxy is at a significant distance from us.
