The galaxy presents as a largely homogenous, elliptical structure, exhibiting a high degree of central concentration. Its overall shape is consistent with a spheroidal morphology, appearing largely smooth with minimal discernible features. There is a slight color gradient visible, transitioning from a more reddish hue at the center to a somewhat greener tint at the edges. This suggests a population of older, redder stars concentrated in the core, with potentially younger, bluer stars distributed throughout the galaxy's outer regions. The light distribution is relatively uniform, indicating a well-mixed stellar population and suggesting a lack of recent major merger events, although some minor disturbances cannot be ruled out. Based on these observations, the galaxy likely has a significant mass and a modest rate of star formation.
