The galaxy presents a generally smooth morphology with a high degree of central concentration. It has a noticeably elongated shape, resembling a cigar or spindle. The light distribution suggests a higher density of older stars, particularly in the central region, exhibiting a yellowish-orange hue. The color becomes slightly bluer towards the outer regions indicating possible presence of younger stars with ongoing, but potentially low, levels of star formation. There is no evidence of strong spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Minor disturbances cannot be ruled out, however. The object's overall appearance is consistent with an elliptical galaxy.
