The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. Its form is approximately elliptical, trending towards a rounded shape rather than an elongated or cigar-like appearance. The central region displays a brighter, more concentrated luminosity profile, likely indicating a significant stellar population density within the galactic nucleus. A faint, diffuse halo surrounds the core, extending outwards. There are indications of subtle features or possible disk-like structures within the halo, though these are not sharply defined and may be the result of low-level star formation or dust lanes. There are no obvious signs of a major ongoing merger, although there are minor hints of disturbances in the outskirts, possibly related to smaller interactions. Overall, the galaxy appears to be relatively evolved. The color gradients suggest a mix of stellar populations, with potentially older, redder stars concentrated towards the center and slightly bluer populations in the outer regions, implying a declining, but not absent, rate of star formation.
