The galaxy exhibits a relatively smooth morphology. It has a generally rounded shape, with a lack of apparent spiral arm structures or significant asymmetries. There is a clear distinction of at least one of the galaxy's colors, leaning towards a turquoise. This may suggest a population of younger, hotter stars within that part of the galaxy. Another section of the galaxy has more subdued yellow or green colors.

The overall form suggests that this system is a likely evolved galaxy residing at a considerable distance from the observer. The overall form of the galaxy shows little evidence of significant recent or ongoing mergers, and lacks any apparent tidal tails or strongly disrupted structures. However, there might be some minor disturbances occurring.
