The galaxy presents an overall elliptical morphology, appearing moderately rounded with a deviation towards an intermediate shape. The light distribution suggests a smooth profile, with no strong evidence of spiral arms or a well-defined disk structure. There may be subtle signs of a galactic merger, but the overall shape suggests a non-disturbed system. The nucleus is bright, but the magnitude increases when moving away from the central region, and the extended halo shows a diffuse outer structure. Color variations across the galaxy are subtle, with a slightly redder core transitioning to a bluer outer halo.
