The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology without prominent spiral arms or a defined disk structure. The light distribution suggests a high degree of central concentration, with brightness decreasing gradually towards the outer regions. It displays a roughly spherical shape, lacking significant elongation or asymmetry. The galaxy's color suggests a population of primarily older stars, indicated by the yellow-orange hue. There is no evidence of recent star formation, such as blue star clusters or dust lanes. The overall appearance suggests a relatively quiescent galaxy, likely with minimal ongoing star formation and a well-mixed stellar population. There is no observable evidence to suggest any recent or ongoing merger activity or tidal disturbances. The galaxy exhibits a compact structure.
