The galaxy presents as a relatively compact object with an apparent disk structure. Its overall shape is largely smooth and elliptical in appearance, displaying a notable degree of central concentration. The light distribution is relatively even across the body of the galaxy, with a slight color gradient visible from the core outwards. There may be some subtle disturbances or irregularities in its structure suggesting a possible past interaction or merger event. There does not appear to be any dust obscuration. The light emitted indicates a relatively high rate of star formation.
