The galaxy presents a morphology that is largely smooth and featureless. Its light distribution appears to be concentrated towards the center, exhibiting a bright core with a more diffuse halo. There is some slight elongation in its shape, but it appears mostly rounded. Overall the galaxy appears to be a fairly isolated system, with no obvious signs of significant tidal disruption or interaction with other galaxies. There appears to be a secondary point of light, but it may be a star within the galaxy that is particularly bright. The color profile suggests that the galaxy has a population of old stars.
