The galaxy presents a somewhat amorphous morphology, exhibiting a bright central region that appears approximately elliptical. The core is intensely luminous, displaying a concentrated emission profile. This bright central region is surrounded by a more diffuse halo of lower surface brightness. This surrounding halo presents an overall bluish hue, potentially indicative of a population of younger, hotter stars. There is a suggestion of minor structural disturbance or irregularity in the outer regions, possibly indicating interaction with another galaxy. The galaxy’s edge is not sharply defined but rather gradually fades into the background sky. There appears to be some evidence of a ring-like structure or a region of enhanced star formation in the inner region of the halo, displaying a greenish color.
