The galaxy presents as a centrally concentrated system with an apparent smooth morphology. The overall shape is moderately elliptical, showing a slight elongation. The central region exhibits a higher luminosity with a yellow-white hue, possibly indicating a population of older stars. The outer regions appear more diffuse, with a bluer tint, perhaps due to the presence of younger stars and ongoing star formation, though the rate seems relatively low. There are subtle signs of a potential minor disturbance in the galaxy’s structure.
