The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, featureless morphology. There is a dominant, bright central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions appear fainter, with a subtle gradient in color, transitioning towards a slightly redder shade. There is no apparent spiral arm structure or dust lane obscuration visible. The overall light distribution suggests a relatively uniform stellar density that decreases radially from the center. There is little evidence of active star formation, which would have been visible as blue or UV light. No signs of tidal tails or major morphological disturbances are present, suggesting it is not undergoing a major merger event. The galaxy appears relatively isolated.
