The galaxy presents a distinct spiral morphology. Its structure includes a prominent central bulge exhibiting a moderate size relative to the overall disk. Surrounding the bulge, spiral arms are clearly discernible, displaying a tightly wound configuration, with some arms being more distinct than others. There appear to be two main arms. The arms show the presence of active star-forming regions. The overall color of the galaxy suggests a mixed stellar population, with bluer regions likely indicating ongoing or recent star formation and yellower components associated with older stellar populations. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances, although a close inspection suggests that it has potential minor disturbances. A weak bar structure seems to be present across the center of the galaxy. Overall, it appears to be a normal spiral galaxy.