The galaxy presents as a somewhat elongated, diffuse object. The light distribution suggests a relatively smooth structure, lacking prominent spiral arms or a distinct bulge. The primary color appears bluish, hinting at a population of younger, hotter stars. Given the overall smoothness and shape, a classification of elliptical or lenticular galaxy seems plausible. There may be some minor disturbances within the galaxy, although no obvious merger events are visible. Overall, this appears to be a galaxy with a low star formation rate.
