The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The color profile suggests a dominance of older stellar populations, indicated by the redder hue concentrated toward the galactic nucleus, possibly due to a higher density of evolved stars and dust obscuration. Fainter, bluer emission extends outwards from the core, with some indications of a disk-like structure, where star formation might still be present. The galaxy appears to have some slight disturbances or distortions in its overall shape, although it is most likely not in the process of major merger activity. The overall shape appears slightly elongated, exhibiting a minor cigar-shaped morphology rather than being perfectly circular.
