The galaxy appears to be a spiral galaxy, viewed at a relatively high inclination. There is a central bulge that is visible in the centre of the object. The bulge is elongated along what appears to be the major axis of the disk. A prominent, somewhat patchy structure is visible within the disk. The galaxy exhibits a colour gradient, transitioning from bluer hues towards the edges of the disk to redder colours near the central bulge. This may be due to younger populations of stars towards the edges and older populations towards the center, potentially due to ongoing star formation in the outer disk. There is no clear evidence of a major ongoing merger or tidal disruption in this image, although there is evidence of a minor disturbance of the features in the disk. The galaxy has a relatively smooth overall appearance, but with some degree of observed internal structure.
