The galaxy presents as a slightly elongated, disk-shaped structure. A bright, concentrated central bulge is apparent, exhibiting a relatively smooth texture. Faint, diffuse spiral arms appear to emanate from the central bulge. These arms are not sharply defined, showing a somewhat flocculent, less organized structure. The overall color of the galaxy appears to be a pale blue-white, suggesting a moderate level of recent or ongoing star formation. There appears to be some disturbances within the structure of the galaxy, potentially indicating a past or ongoing merger event.
