The observed galaxy presents a morphology consistent with a spiral galaxy, with a prominent central bulge and a relatively well-defined disk. The spiral arms appear somewhat loosely wound. The galaxy is observed close to face-on, permitting a relatively clear view of the spiral structure. A potential bar structure may be present, though not particularly prominent. Star formation appears present in the arms, but not exceptionally vigorous. There may be some minor disturbances, suggesting past or ongoing interactions. The central bulge has a color suggesting a slightly older stellar population compared to the disk. Overall, the galaxy presents as a fairly typical spiral galaxy undergoing normal evolutionary processes.
