The galaxy presents a largely smooth, elliptical morphology, with a concentrated central bulge that is yellowish in color. This suggests an older stellar population dominates the bulge. A fainter, greenish hue is present around the core, which could indicate some ongoing, albeit limited, star formation activity. There is no obvious spiral structure or bar. The shape appears nearly round, with no significant elongation or distortion. There is no visible evidence of tidal tails, major mergers, or strong gravitational disturbances, suggesting it is a relatively isolated system that is in a late stage of its evolution. 
