The galaxy appears to be a spiral type, though with a somewhat less defined structure. A central bulge is noticeable, exhibiting a bright, concentrated luminosity. Faint, diffuse spiral arms extend outwards from the bulge, showing hints of blue hues. A dust lane may be present along one edge, obscuring some of the galactic disc. The overall morphology is not highly disturbed, suggesting no recent major merger events. The galaxy is moderately sized. Star formation is present, but does not appear highly active.
