The galaxy presents a largely smooth morphology, appearing as a somewhat rounded, though not perfectly spherical, structure. A central, bright region is prominent, exhibiting a yellowish hue, potentially indicating an older stellar population or dust obscuration. This central region transitions into a more diffuse halo or disk component characterized by a greenish tint. There is some suggestion of a very slight disturbance in the outer regions, however it otherwise exhibits little evidence of significant tidal interactions or mergers. The overall color profile suggests a mix of stellar populations, with potentially subdued star formation. The galaxy shows no obvious spiral arm structure or distinct features associated with active galactic nuclei at this resolution.
