The galaxy appears to be a luminous object, exhibiting a generally smooth morphology. It has a round, elliptical shape. The light distribution is relatively even across the galactic body, with a concentration toward the center. There appears to be minimal structural disturbance or signs of ongoing major mergers. There is a very slight hint of bluer color in certain areas. The object's color suggests a substantial population of older stars, with the potential for ongoing star formation at a moderate rate.
