The galaxy presents as a smooth, elongated structure. Its color profile transitions from a more concentrated, yellowish core to a bluer hue at its outer edges. There is a slight asymmetry, as one side extends further and appears more diffuse compared to the other, creating a cigar-like shape. No distinct spiral arms or bar features are visible. The morphology is indicative of an elliptical or lenticular galaxy, with a relatively old stellar population contributing to its overall color. The structure is not disrupted, which suggests it is likely a relaxed system that is not currently undergoing a major merger. A subtle distortion or asymmetry could point to past interactions or minor disturbances. Overall, the galaxy appears to be a relatively evolved system with a moderate mass.
