The galaxy exhibits a roughly elliptical morphology, appearing somewhat elongated. It presents a smooth, featureless disk, with no distinct spiral arms or bar structure readily apparent. The central region displays a bright core, suggesting a concentration of stars. The color distribution shows a general trend of bluer hues extending outward from the central region, with the core itself appearing slightly redder. This could indicate younger stellar populations in the outer disk compared to the core. There is evidence of some minor disturbances or irregularities in the galaxy's structure.
