The galaxy presents as a spiral type, with a noticeable disk structure. Spiral arms are visible, exhibiting a somewhat patchy and flocculent morphology. There is a central bulge that is neither overly dominant nor negligible, appearing to be of moderate size within the overall galactic structure. The galaxy does not appear to be perfectly face-on; there is a slight tilt in its orientation relative to our line of sight. The disk appears to be somewhat disturbed, indicating potential interactions or mergers. The presence of luminous regions suggests active star formation.
