The galaxy presents a roughly elliptical morphology, with a notable extension along one axis, suggestive of a cigar shape. A significant portion of its light appears relatively smooth and homogenous. The color gradient transitions from a redder hue at one end, to a bluer hue towards the opposite extremity. The redder portion appears more concentrated, while the bluer region is more diffuse. There is a subtle hint of possible disturbed morphology, potentially indicative of a minor interaction or merging event. Overall, the galaxy appears to be a massive system exhibiting relatively low star formation.
