The galaxy presents as a relatively smooth, elliptical object, elongated in shape with an approximate aspect ratio of 3:1. The color profile appears largely uniform, with a subtle concentration of bluer light towards the core regions, suggesting some level of ongoing, though not necessarily intense, star formation. A hint of a yellowish tint is visible on one side, possibly indicating a pocket of older stellar populations or dust obscuration. The overall smooth appearance and lack of pronounced spiral arms or significant dust lanes suggests that this is likely a relatively old and evolved system. There is no evidence of a major ongoing merger or significant tidal disturbances.
