The galaxy exhibits a spiral morphology, with discernible, albeit somewhat tightly wound, spiral arms emanating from a central bulge. The bulge appears moderately prominent. The spiral arms showcase a distinct blue hue, suggestive of ongoing star formation activity. The overall structure indicates a relatively high probability of being a non-edge-on disk galaxy. There is a likelihood of minor disturbance of some sort, but the galaxy does not appear to be undergoing a major merger currently. A bar structure is weakly indicated within the central region, but it is not strongly defined. The central region displays a yellowish coloration.
