The galaxy presents as a centrally concentrated object with a generally smooth morphology. It has a shape that is somewhere between round and elliptical, with a slight elongation. There is some indication of possible minor disturbances in the overall structure, but the primary form remains relatively undisturbed. The galaxy exhibits a dominant smooth component, suggesting an absence of well-defined spiral arms or a prominent disk-like structure. The color profile indicates a more substantial presence of older stellar populations, corresponding to a weak amount of star formation activity. Based on the object's size and estimated distance, it can be classified as a relatively massive galaxy.
