The galaxy presents a predominantly bluish hue, suggesting active star formation. Spiral arms appear to emanate from a central bulge. The presence of these arms indicates ongoing dynamic activity and potential gravitational interactions within the galactic structure. The bulge is moderately sized, possibly indicative of an older stellar population concentrated toward the galactic center. There is no indication of a particularly active galactic nucleus. A subtle bar-like structure is suspected through the center. There does not appear to be any major disturbances, though it could be undergoing a minor merger. Overall, the galaxy is likely a spiral galaxy with intermediate mass, experiencing moderate levels of star formation.
