The galaxy presents a clear spiral structure. Two well-defined spiral arms are prominent, exhibiting a loose winding pattern. The central bulge appears moderately sized, with a yellowish hue, suggesting an older stellar population. There may be a weak bar structure extending from the central bulge. Star formation appears to be present, but the spiral arms are not particularly knotty or blue, indicating moderate star formation activity. No signs of significant tidal disturbances or ongoing major merger events are readily apparent, although minor interactions cannot be ruled out. The galaxy is tilted, and the disk appears to be seen at an intermediate angle, neither face-on nor edge-on.
