The galaxy presents a predominantly blue hue, suggestive of ongoing star formation. Its morphology appears as a spiral galaxy, with loosely defined spiral arms emanating from a central region. The arms exhibit a clumpy structure, possibly indicating regions of active star birth. The central bulge is comparatively small, and the disk structure appears to be the dominant feature. No significant bar structure is visually apparent. There is some evidence of minor disturbances within the galaxy, but there are no signs of it merging with another galaxy. It is not edge on. The galaxy appears smooth but it definitely has features.
