The galaxy presents as a spiral with a notable central bulge that appears yellowish, likely indicative of an older stellar population. The spiral arms are tightly wound and moderately defined, exhibiting a bluer hue suggesting regions of active star formation. There is evidence of multiple spiral arms, possibly three or four. The galaxy shows no signs of a strong bar structure. The overall morphology suggests a classification leaning towards an intermediate spiral type, with a relatively well-defined bulge and tightly wound arms. The galaxy is not experiencing any major mergers or disturbances, and the disk of the galaxy is oriented somewhat face-on.
