This galaxy presents as a spiral type, viewed at an angle oblique to face-on, but not quite edge-on. The central bulge region appears prominent and moderately sized, exhibiting a yellowish-white color, indicative of an older stellar population. Faint spiral arms are visible, exhibiting a somewhat patchy distribution. The arms appear bluer in color, suggesting active star formation within. The disk of the galaxy is relatively smooth, with some signs of disturbances. There is no clear evidence of a strong bar structure. Overall, the galaxy exhibits signs of ongoing star formation activity and is likely undergoing some minor interactions based on the slightly disturbed disk.
