The galaxy presents as a diffuse object with a relatively compact core. The overall color is suggestive of older stellar populations. There appears to be some faint disk structure with possible spiral arms emanating from the central bulge, though the morphology is heavily disturbed. There are no clear signs of recent or ongoing star formation within the galaxy itself. The object does not appear to be interacting with any other galaxies, though there may be some small disturbances in the morphology of the galaxy, which could indicate an earlier minor merger event.
