The galaxy presents as a centrally concentrated, elliptical-like system with a smooth, diffuse appearance. The dominant color is a yellow-white hue, suggesting a population of older stars. There appears to be a slight asymmetry in the light distribution, potentially indicating a minor interaction or disturbance. A hint of bluer light is visible on the periphery of the galaxy on the left side, possibly indicating the presence of some younger stars in that area. There is no clear evidence of spiral arms or a prominent disk. The overall morphology suggests a galaxy that is undergoing minimal current star formation, with a significant fraction of its stellar mass already formed. The galaxy exhibits a moderate level of luminosity, consistent with a galaxy of intermediate mass.
