The galaxy appears as a diffuse, centrally concentrated object. It exhibits a subtle disk-like structure, though this is somewhat obscured by its low surface brightness and faintness. There are faint signs of spiral arms or irregular patches within the disk, with what appear to be regions of star formation. The color profile seems to indicate the presence of both older stellar populations as well as bluer star forming regions within the spiral arms. There is no apparent nucleus or bar structure. Overall, the galaxy appears to be a fairly average spiral or possibly an irregular disk galaxy at a moderate distance, without any signs of active galactic nuclei or major interactions.
