The galaxy presents as a somewhat elliptical, though nearly round, structure. Its core is a bright, concentrated yellow-white. The color profile suggests a population of older stars, possibly within a bulge. Moving outward from the core, a more diffuse region of lower surface brightness is observed. Hints of bluer light are present in the outer regions, indicative of younger stellar populations and potential ongoing star formation. Irregularities or minor disturbances in the galaxy's form might exist, especially in the fainter outer regions. Overall, it appears to be a fairly massive galaxy with a relatively smooth texture.
