The galaxy presents as a moderately inclined, disk-like structure with a relatively smooth overall appearance. There are faint features visible that could be indicative of internal structure. It exhibits a somewhat elongated morphology. The light distribution suggests a possible central concentration. The object displays a subtle blue hue in its central region, with a slightly redder coloration in the outer edges of the disk. There may be some evidence of minor gravitational disturbance in its morphology. There appear to be little to no signs of any ongoing merger activity, but there may be some minor disturbances within the structure. The galaxy appears to be a relatively quiescent system.