The galaxy exhibits a disk-like morphology, although the angle of observation obscures a clear assessment of its spiral structure. Faint arms appear to be present, extending outwards from a central bulge region. The central bulge is not particularly prominent. Color gradients across the galaxy suggest ongoing star formation, with bluer hues concentrated in the outer regions of the disk, potentially indicating younger stellar populations. The central region is characterized by yellower and redder hues that may suggest the presence of older, cooler stars. There is no indication of a dominant bar structure. There is no evidence of any major merging activity, although there are some minor disturbances within the galaxy.