The galaxy presents a somewhat amorphous shape, appearing largely as a central concentration of light with some extended, diffuse features. The color is predominantly bluish, suggestive of a stellar population with relatively young, hot stars. There is a degree of irregularity observed, potentially indicating on-going or recent interactions or mergers. The overall appearance is neither that of a pure elliptical galaxy nor a well-defined spiral, but rather something in between, leaning towards a disturbed morphology. Evidence of interaction or a merger is suggested by a somewhat irregular light distribution and morphological disturbances. There are brighter areas of the galaxy which may be associated with star forming regions.
