The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. There is a noticeable color gradient, transitioning from a yellowish-white core to a redder outer region, suggesting an older stellar population dominating the central bulge and possibly some ongoing star formation or a younger population present in the outer disk. The galaxy appears to be viewed at a slight inclination, as its shape is not perfectly circular, but rather elongated. No distinct spiral arm structures or prominent dust lanes are visible, indicating a disk galaxy with weak or absent spiral structure. The galaxy appears to be relatively isolated, with no obvious signs of recent major mergers or tidal disturbances. A small feature to the right appears to show a merging, but it is minor. Overall, the object appears to be a fairly typical elliptical galaxy with an estimated stellar mass of approximately 10^10 to 10^11 solar masses, observed at a redshift of approximately 0.12. Given the low star-formation rate, star formation may have subsided within the galaxy.
