The galaxy presents a somewhat amorphous morphology, displaying a mix of smooth and potentially disturbed features. A central concentration of light suggests the presence of a bulge or core region, exhibiting a yellowish hue. To one side, there appears to be a region with a bluer color, possibly indicating areas of active star formation. The galaxy's overall shape is more rounded than elongated, but there are subtle asymmetries that could point toward interactions or internal disturbances. There seems to be an absence of defined spiral arms or a distinct disk-like structure, leading to the possibility that this may be an elliptical galaxy, or a spiral that has been distorted due to interactions. The object appears to be experiencing a relatively low rate of star formation. It may be undergoing or have undergone a merging event.
