The galaxy appears to be a relatively small, low-mass system, likely a dwarf galaxy at a moderate distance. Morphologically, it appears to be a disk galaxy. It has a relatively smooth light distribution. A slight elongation suggests it may not be perfectly spherical. It shows hints of spiral arm structures and areas of active star formation. There is a subtle color gradient, with a slightly bluer hue, indicating the presence of younger stellar populations. This color suggests modest star formation, though the overall rates seem to be relatively low. There are no obvious signs of major disturbances or interactions, though a minor disturbance cannot be fully ruled out.
