The galaxy presents as a lenticular or possibly a spiral galaxy seen at a relatively high inclination. There is a bright central bulge that dominates the galaxy's luminosity, surrounded by a flattened, fainter disk. The disk shows hints of spiral structure, but these are not well-defined, suggesting a relatively smooth stellar distribution. The color of the galaxy appears to be trending towards the redder end of the spectrum suggesting an older stellar population. There are no indications of active star formation regions in the disk. The overall appearance points towards a galaxy that is in a more evolved state. It appears that this galaxy is an isolated system, with no other galaxies nearby that could be interacting with it.
