The galaxy exhibits an elliptical morphology, appearing predominantly smooth in structure. The core region shows a concentrated, bright yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, the color gradually shifts towards a more diffuse greenish-yellow, suggesting a mix of stellar ages or perhaps the presence of some ongoing, though limited, star formation in the outer regions. The overall shape is somewhat elongated, deviating slightly from a perfectly circular form. There's no clear evidence of significant spiral arms, bars, or tidal disturbances, suggesting it is a relatively isolated system that is not currently undergoing a major merger event. The galaxy appears to be in a relatively quiescent state.
