The galaxy appears as a somewhat elliptical, diffuse object. The central region is brighter and more concentrated, suggesting a bulge component. Fainter, elongated structures extend from either side of this central region, suggestive of a disk. The disk exhibits a smooth texture with no clear spiral arm definition discernible in this image. The overall color is slightly redder, particularly concentrated in the central bulge, suggesting an older stellar population. There is subtle evidence of some disturbances or asymmetry within the disk and at the edges of the galaxy, which may be indicative of tidal interactions or past merger events.
