The galaxy presents a predominantly smooth morphology, exhibiting a bright, concentrated central bulge. There is a faint disk-like structure surrounding the bulge, showing some indications of spiral arms. The color gradient suggests a relatively evolved stellar population, with a redder central region and bluer, younger stars sparsely populating the outer disk. There is a slight distortion in the galaxy's shape, possibly indicating a minor gravitational interaction or disturbance. Overall, the galaxy appears to be a transition type, perhaps between a spiral and lenticular galaxy, with subdued star formation activity.
