The galaxy appears to be a spiral galaxy with a fairly prominent central bulge. The arms are tightly wound, displaying a flocculent structure with several identifiable arm segments. There is an indication of a possible bar feature within the central region of the galaxy, though this is not definitive. The galaxy appears moderately inclined to our line of sight. The color distribution indicates a population of older stars dominating the bulge, with bluer regions apparent in the spiral arms, suggesting ongoing star formation. The morphology indicates a system that is not undergoing a major merging event, although some minor disturbances in the arm structure may suggest a previous interaction or ongoing accretion. The overall light distribution appears smooth, with no significant dust lanes or other irregularities visible at this resolution.