The galaxy presents a roughly elliptical morphology. The central region exhibits high surface brightness and appears primarily white, suggesting a concentration of older stellar populations. Moving outwards, a distinct redder ring surrounds the bright core, likely indicating a population of dust and cooler stars. Fainter, bluer regions are present within the inner area, which could point to areas of on-going or recent star formation. The outer edges of the galaxy fade gradually into the background sky. Evidence of disturbance within the galaxy's morphology is indicated by some asymmetrical features, possibly due to minor gravitational interaction or internal dynamics.
