This galaxy presents as a somewhat irregular, roughly elliptical shape. The central region exhibits a high surface brightness, appearing nearly white, likely indicative of a concentrated stellar population and potentially an active galactic nucleus. Surrounding this bright core is a less intense, more diffuse region of blue light. This blue light could be attributed to recent star formation within the galaxy's disk. There is a subtle indication of disrupted spiral arm structures, or perhaps tidal debris, that is likely due to some type of gravitational disturbance. 
