The galaxy presents as a somewhat asymmetrical structure, with a luminous core region. There is an extended halo or envelope of light, and the galaxy appears relatively smooth, and has a moderate color gradient, transitioning from a bluer hue toward the outer edges to slightly redder tones near the center. There is some evidence of minor disturbances or interactions that would likely involve tidal forces, or past mergers. Overall, the object displays a morphology characteristic of a fairly evolved galaxy with a significant stellar mass.
