The galaxy presents a generally smooth morphology, appearing elliptical in shape with a high degree of roundness. There is a subtle color gradient visible, with the central regions appearing slightly more reddish-yellow than the outer edges, which tend towards blue. This could indicate older stellar populations concentrated in the core. No distinct spiral arms or strong features are readily apparent, and there's a lack of significant dust lanes or major disturbances in its structure. There may be very minor disturbances, but it could just be the limitations of the resolution in this image. The galaxy does not appear to be undergoing a major merger.
