The galaxy exhibits a morphology that is largely smooth and elliptical in appearance. The galaxy displays an intermediate roundness, leaning more towards an elliptical than a spherical shape. There is a bright central bulge, indicating a concentration of older stars in the galactic nucleus. Fainter blue hues are observed at the outer edges of the galaxy, suggesting ongoing star formation within the galactic disk. There is a potential indication of a minor disturbance in the galaxy's structure.
