This galaxy exhibits a morphology that appears to be predominantly smooth, with a slight elongation. The central region of the galaxy presents a bright, concentrated luminosity, likely indicating a dense stellar population or an active galactic nucleus. There is some evidence of a disk-like structure or faint arms, though these features are not sharply defined. A blue hue is perceptible in the outer regions, suggesting the presence of younger stars and ongoing star formation within the galaxy. Overall, the galaxy displays characteristics intermediate between a pure elliptical and a spiral galaxy, possibly a lenticular galaxy or a spiral galaxy with tightly wound arms. There may be some minor gravitational disturbance from a past merger.
