The galaxy presents a primarily smooth morphology, with a notable absence of distinct spiral arms or a well-defined disk structure. The overall shape is somewhere between round and slightly elongated. There may be only minor signs of disturbances. The galaxy exhibits a color gradient, appearing bluer towards the center and redder in the outer regions. This may indicate older stellar populations inhabiting the outer regions. The redder hue could also be caused by dust extinction. The relative lack of blue light suggests that star formation may be moderate. Overall, this is a galaxy in a middle stage of it's life.
