The galaxy presents as a somewhat elongated, elliptical form with a centrally concentrated bulge. The light distribution appears relatively smooth, with a gradual decline in brightness from the core outwards. There is a faint, diffuse halo surrounding the main body of the galaxy. The color profile suggests a population of older stars, with a reddish tinge towards the core and a slightly bluer hue in the outer regions, implying ongoing, albeit modest, star formation. No obvious spiral arm structures or dust lanes are apparent. The overall morphology indicates a galaxy that has likely undergone significant evolutionary processes. The lack of major disturbances suggests a stable, isolated system or one that has completed a merging event in the distant past.
