The galaxy presents as a largely homogenous spheroid with a high degree of central concentration. The primary color is a yellow-orange hue, suggesting an older stellar population. There is subtle color variation in the outer regions, with some hints of green, possibly indicating areas of residual star formation, though the overall star formation rate appears low. The morphology is generally smooth, without any readily apparent spiral arms, bars, or significant tidal features indicative of recent or ongoing mergers. The shape is predominantly round, showing minimal elongation. The galaxy's size is relatively compact. 
