The galaxy presents as a relatively smooth, elliptical morphology. There is a slight elongation, but it is predominantly round in appearance. The light distribution appears concentrated towards the center, suggesting a prominent galactic bulge. There is little evidence of spiral arm structure or significant dust lanes within this system. The overall color is slightly yellow and could indicate a population of older stars, suggesting a potential low star formation rate. There might be some evidence of minor tidal disturbances, but the galaxy appears to be mostly isolated.
