The galaxy presents as a relatively compact, elliptical or lenticular system. Its overall color appears to be predominantly yellow, suggesting an older stellar population with fewer hot, young, blue stars. The light distribution appears smooth and centrally concentrated, with no obvious spiral arm structure or prominent dust lanes visible in this image. It exhibits a high degree of roundness, with a minor suggestion of deviation from perfect circularity. There is no immediately apparent sign of ongoing major merger activity or significant tidal disturbance in this image; however, minor disturbances are still possible. Star formation appears to be largely quiescent. Based on its color and morphology, this galaxy is likely a relatively massive system.
