The galaxy presents as a relatively smooth and centrally concentrated system. The overall morphology appears elliptical or lenticular, exhibiting a high degree of central symmetry with no prominent spiral arm structures or dust lanes visible. The color gradient suggests a population of older stars, contributing to the overall redder hue, particularly prominent toward the center. There is a subtle green/blue tint on the periphery, indicating the presence of a minor population of younger stars. There is no indication of a significant ongoing merger, although there appears to be a faint point of light on the right that could be a part of the galaxy.
