The galaxy presents as a moderately luminous object, exhibiting a central concentration of light that graduates outward. The core region appears to be composed of older stellar populations, indicated by its redder hue. Moving outward from this core, the luminosity decreases, with suggestions of somewhat diffuse, disk-like morphology. The morphology of this object is suggestive of a spiral galaxy, but the features are indistinct. There appears to be some indication of a minor interaction or disturbance in the upper regions of the galaxy.
