The galaxy appears as a single, relatively smooth object. There is a slight elongation in its shape, deviating from a perfectly circular morphology. Its color profile shows a concentration in the redder wavelengths with a possible hint of light emission in the bluer wavelengths in its outer regions. No distinct spiral arm structures are apparent. There is evidence of disturbed morphology possibly indicative of a recent or ongoing merger event. There may be possible tidal tail remnants in some areas of the outer regions of the galaxy.
