The galaxy presents an overall amorphous shape, with a relatively smooth appearance. It appears moderately compact and relatively small. There is a slightly concentrated central region, from which light diffuses outwards. There are some hints of a disk or arm-like structure but the morphology is largely irregular. A fraction of the galaxy appears featureless. There are a few distinct regions exhibiting a redder hue, which may indicate areas of active star formation or older stellar populations within dusty environments. There is no obvious indication of a major merger event, although a minor disturbance may be present. The color gradients observed suggest a non-uniform distribution of stellar populations and dust content across the galaxy.
