The galaxy presents a generally smooth morphology with some features. The object exhibits an elongated, cigar-like shape. The central region appears brighter and whiter, possibly indicating a concentration of older stars, while the outer regions appear less luminous. The presence of disk-like components suggest the possibility of rotation. Given the disk-like appearance and the observed color gradients, this galaxy may be actively forming stars. The relatively high star formation rate suggest this is not a quiescent galaxy. There is no clear evidence of a major merger event, but some minor disturbances or tidal features may be present.
