This galaxy presents as a somewhat diffuse object with an approximate diameter of 4.1 kiloparsecs. It exhibits a moderately smooth morphology, with some evidence of possible disturbances. The light distribution suggests a central concentration, though not particularly pronounced. The galaxy appears elongated, exhibiting a slight cigar shape. There is a possible minor disturbance with a low probability of this galaxy merging with another galaxy. Color gradients suggest a redder core, possibly indicating an older stellar population. Overall, the galaxy appears to be undergoing moderate star formation.
