The galaxy exhibits a clear disk structure, viewed at an angle that is close to face-on. Distinct spiral arms are observed, appearing tightly wound around a prominent central bulge. The bulge is approximately moderate in size, exhibiting a yellowish color, likely indicative of an older stellar population. The spiral arms appear as a bluish color, and areas of ongoing star formation are suspected. The dust lanes are difficult to observe at this resolution. Overall, the galaxy does not appear to be significantly disturbed or undergoing a major merger event.
