The galaxy exhibits an elliptical morphology, with a generally smooth appearance, though some distortions are visible. The shape appears to be in between round and cigar-shaped. There is evidence of a potential merger event or gravitational disturbance, with the suggestion of tidal tails or disrupted structures emanating from the central region. The color gradient transitions from a bluer hue in the outer regions to a more yellow/red color in the galactic core, suggestive of older stellar populations concentrated towards the center and younger stars in the outer disk. Overall, it suggests a galaxy with a considerable stellar mass.
