The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of roundness. There is an absence of clear spiral arm structures or a well-defined disk. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus. The color appears largely uniform across the galaxy.

Based on its color and smooth morphology, it seems to contain a population of older stars. There seems to be little indication of active star formation within the galaxy. There also appears to be no evidence of recent or ongoing merger activity. 