The galaxy presents as a small, relatively faint object, exhibiting a slightly irregular morphology. There is a distinct blue-ish central concentration of light, which may indicate a region of active star formation. The overall shape is neither perfectly elliptical nor a well-defined spiral, leaning toward a more amorphous structure. The presence of some irregularities suggests possible interactions or disturbances that are causing the somewhat distorted shape. Additionally, there is a hint of what may be a disk-like structure, but it is not well defined. The light from the galaxy is dim, potentially indicating it is older or not actively forming a large number of stars in total. The overall impression is that of a galaxy undergoing some form of morphological transformation or interaction, potentially with a merging event.
