The galaxy presents a primarily blue hue, indicative of ongoing star formation. While the image quality limits detailed morphological classification, there are hints of a possible disk structure. The overall appearance suggests a galaxy with a relatively late-type morphology, possibly a spiral or irregular galaxy. There appears to be some low level of disturbance to the general form of the galaxy. There is a somewhat amorphous shape, possibly indicating recent or ongoing minor merger activity influencing its structure. The approximate diameter is approximately 5 kpc.
