The galaxy presents as a face-on or near face-on spiral galaxy. The central bulge region exhibits a bright, concentrated luminosity, appearing yellow-white in color, suggesting an older stellar population. Fainter spiral arms extend from the central region, exhibiting a bluer hue, indicative of ongoing star formation. The overall structure appears somewhat flocculent. The disk component is evident but not sharply defined. The galaxy demonstrates a moderate degree of ellipticity. There is no clear evidence of a strong central bar structure. There is no indication of a major ongoing merger. There is a slight irregularity in the outer regions of the disk, suggesting a potential minor disturbance or interaction.
