The galaxy presents as a largely smooth, elliptical-like structure. It displays a concentrated central bulge with a yellowish hue, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes. The overall color gradient transitions subtly from a yellowish core to a redder periphery, indicating a potential variation in stellar age and composition across the galaxy. The galaxy appears moderately luminous, and is not perfectly round. There may be a faint tidal tail or minor disturbance, but it is difficult to tell at this resolution.
