The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It is fairly compact, with a central concentration of light that dominates the overall appearance. The core region appears smooth, with a diffuse halo of light extending outwards. This halo is not uniformly distributed, showing some irregularities and hints of potential features. There is a discernible reddish area located off-center, possibly indicative of dust obscuration or a region of intense star formation. Overall, the galaxy's structure suggests a system where the light is dominated by older stellar populations, but with hints of ongoing or recent star-forming activity. It does not show any clear signs of a major ongoing merger, though subtle disturbances in the outer regions cannot be ruled out.
