This galaxy presents a flattened, elliptical morphology. Its structure appears largely smooth and concentrated, with a high degree of central luminosity. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue at its outer edges to a warmer, yellower tone towards the core. This suggests a potential difference in stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars populating the disk. There is no obvious indication of spiral arms or significant dust lanes. Based on the axial ratio, the galaxy is likely an elliptical, but may potentially be a lenticular type seen at a high inclination angle. There is no clear visual evidence of a recent or ongoing major merger, though there is the possibility of faint minor tidal features that suggest the presence of minor disturbance of the system.
