The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. It displays a yellowish hue, suggesting an older stellar population with fewer young, hot stars. The galaxy appears nearly spherical, with minimal apparent disk features. The light distribution is relatively even, fading gradually from the bright core to the outer regions. There is some subtle color variation throughout the galaxy, the central portion appearing more intensely yellow than the peripheral areas. There is no evidence of active star formation regions or prominent dust lanes. Furthermore, there is no clear indication of recent merger activity or significant tidal disturbances, indicating a relaxed morphology.
