The galaxy appears as a relatively smooth object with a near-circular morphology. The color profile suggests an older stellar population, with a noticeable absence of strong blue emission indicative of active, recent star formation. There is an indication of a slight deviation from perfect smoothness, with a hint of a feature or disturbance, although it is not distinctly defined. The central region appears slightly more concentrated than the outer regions, suggesting a possible bulge component. Overall, the galaxy presents the characteristics of a relatively evolved system.
