The galaxy presents as a grand design spiral galaxy, exhibiting a prominent disk structure. Two well-defined spiral arms emanate from a moderately sized central bulge. The arms are tightly wound and demonstrate a relatively symmetrical structure. Star formation appears to be ongoing within the spiral arms, indicated by the presence of bluish regions indicative of younger, hotter stars. There are hints of a weak bar structure bisecting the bulge. The central bulge shows a yellowish hue, suggesting an older stellar population. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances.
