The galaxy appears to be a relatively smooth, centrally concentrated system. Its light profile suggests an elliptical morphology, with a high degree of roundness. The color is primarily blue-white, indicating a stellar population that includes younger, hotter stars, although this color may also be influenced by redshift. There may be some minor disturbances or interactions indicated by subtle asymmetries or irregularities in its outer regions. The galaxy's overall structure does not suggest a recent major merger event. It is a medium sized galaxy with low star formation.