The galaxy presents as a disk galaxy, viewed at a moderate inclination. It exhibits a bright central bulge that is yellowish in color, suggesting a relatively older stellar population. The disk appears to be somewhat flocculent, with hints of spiral arm structure that are not sharply defined. There is some evidence of ongoing star formation activity, particularly in the outer regions of the disk, as indicated by bluer hues. The overall form shows a possible indication of a tidal interaction or minor disturbance, though the image quality is not sufficient to make a definitive statement.
