The galaxy exhibits a predominantly smooth morphology. Its overall shape appears somewhat elliptical, with a moderate degree of roundness. There are no discernible spiral arms or a prominent disk structure. The light distribution is concentrated towards the center, suggesting a prominent bulge. No major interactions or mergers are clearly evident, though subtle signs of minor tidal disturbances or faint features can not be ruled out. The galaxy's color index indicates that the light is redder suggesting a population of older stars.
