The galaxy presents a somewhat irregular morphology. It appears to be a spiral galaxy seen at a moderately inclined angle. The central bulge is not very prominent, appearing diffuse and only slightly more concentrated than the rest of the galaxy. The spiral arms are not well-defined. A significant portion of the galaxy's light emanates from patchy, clumpy regions distributed throughout the disk, suggesting ongoing star formation. These regions exhibit a bluish tint, likely due to the presence of young, hot stars. There seems to be some tidal features present and some distortions in its shape, possibly indicating a past or ongoing minor merger event. There seems to be some redder regions as well, possibly caused by dust obscuring star formation activity.
