The galaxy presents a somewhat elongated, disk-like morphology. Its light profile appears largely smooth, exhibiting a centrally concentrated brightness distribution that gradually fades outwards. I am unable to discern any distinct spiral arm structures or well-defined dust lanes. The galaxy's color profile exhibits a subtle gradient, appearing slightly bluer at the outer edges of the disk and gradually shifting towards redder hues in the central regions. This is a possible indication of ongoing star formation occurring within the galaxy. I would classify this galaxy as a late-type spiral, likely undergoing a merger. There appear to be a few areas of disturbance.
