The galaxy appears to be a relatively smooth, elliptical type with a high degree of central concentration. The color gradient suggests an older stellar population. The core exhibits a yellowish-orange hue, indicative of evolved stars. The outer regions transition to a slightly bluer color, suggesting a small amount of younger stars. There is no apparent spiral structure or prominent dust lanes. The overall morphology indicates a lack of significant recent merger activity or tidal disturbances. The galaxy exhibits a generally round shape. 
