The galaxy presents as a somewhat diffuse, elongated structure. There is a suggestion of a disk-like component viewed at a high inclination, possibly nearing edge-on. Faint bluer light extends from the central region, suggestive of some star formation. There also appears to be some evidence of tidal disturbances or possible merger activity. The morphological features appear to have moderate levels of disturbance. The central regions exhibit a subtle concentration of light. Overall, the galaxy has a relatively low surface brightness.
