The galaxy presents as two distinct, luminous concentrations of light, suggesting a binary or merging system. The primary component appears nearly spherical, exhibiting a smooth, centrally concentrated morphology. The luminosity profile appears to gradually decrease from the core outwards. The secondary component is similar in appearance but slightly less luminous. There is some evidence of a faint tidal feature that could be a bridge of matter or possibly a minor disturbance between the two galaxies, yet the system is not fully merged. The system has a slightly yellowish hue indicating an older population of stars in the combined galaxy.
