The galaxy presents as a spiral morphology, with a well-defined disk structure. Spiral arms are readily apparent, exhibiting a tightly wound configuration, with the majority of the arms unable to be clearly counted. Star formation appears ongoing, as evidenced by the blue color in the spiral arms. The central bulge is compact and moderate in size, displaying a yellowish hue indicative of an older stellar population. A bar structure is not strongly evident, though a weak bar may exist. No major interactions or mergers are immediately obvious, although minor disturbances can not be ruled out. The disk is oriented close to face-on, with minimal inclination.
