The galaxy presents an elongated, spindle-like morphology, suggesting it is likely an edge-on disk galaxy. The central bulge region appears yellowish, indicative of an older stellar population and lower levels of current star formation. Fainter blue hues are visible along the edges of the disk, possibly representing regions of ongoing star formation within the spiral arms, which appear tightly wound. The overall smoothness of the light distribution implies a relatively undisturbed structure, with no obvious signs of a recent major merger event. The galaxy is a considerable distance away, and its light reveals its star formation rate is substantial, yet the galaxy is unlikely to experience any major merging events with other galaxies. It is an average-sized galaxy.