The galaxy appears relatively compact, with an approximate angular radius around 6 arcseconds. Visually, it exhibits a complex morphology, with evidence of a possibly ongoing or recent interaction. The central region appears somewhat smooth, surrounded by a fainter, more irregular extended structure. There is some asymmetry observed in the outer regions, and may be evidence of tidal features or disrupted arms. Some areas of slightly increased intensity and non-uniform color distribution may be suggestive of star forming regions. The galaxy shows a higher flux in the redder bands, indicating that it could be a more evolved system or one with significant dust obscuration. Overall, the galaxy appears to be undergoing some form of dynamical disturbance or morphological transformation.
