The galaxy exhibits a generally smooth morphology, with a concentration of light towards the center, suggesting a dominant bulge component. The overall shape is elliptical, though not perfectly round. The galaxy has a yellow-orange hue, potentially indicating an older stellar population with relatively low ongoing star formation. There is no prominent disk structure visible, nor are there any clear signs of spiral arms. There might be a very slight indication of minor disturbances in the galaxy's structure, although no major merger events are apparent. Overall, the galaxy appears to be an elliptical galaxy with a largely quiescent star formation rate.
