The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its appearance is largely elliptical. Some subtle, fainter features hint at the presence of a disk or spiral structure, but these are not prominent. The light distribution suggests that it is primarily a spheroid-dominated system. The central region of the galaxy is yellowish-white, which suggests an older stellar population. Bluer hues extend outwards from the core, implying younger stellar populations or star formation. There is no evidence of major mergers or tidal disturbances, although some minor irregularities are apparent. 
