The galaxy presents as an elongated structure, appearing predominantly smooth in texture. The color profile shows a yellow core that seems to transition outwards to a slight green hue at its edges, indicating a range in stellar populations and potential differences in age or metallicity across the galaxy. The morphology leans towards a elliptical or lenticular, but not quite a disk shape. Possible minor disturbances in the structure, such as warping or subtle asymmetrical features, may suggest a past or ongoing gravitational interaction. There is no indication of a recent major merger, or complete disruption of the structure.
