The galaxy appears as a relatively small and faint object. Morphologically, there is a suggestion of a central concentration, but no distinct nucleus is readily apparent. There is some faint, diffuse light surrounding this central area that may indicate a disk component. The image suggests that the galaxy might have undergone some sort of interaction or disturbance. While there are no large tidal tails or other obvious signs of a major merger, there seems to be some asymmetries. The color profile appears reddish.
