The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity, appearing as a bright, yellowish-white core. Moving outwards, the luminosity gradually decreases, fading into a less defined halo with a subtly reddish hue. The galaxy appears relatively undisturbed, without any obvious signs of ongoing mergers or major tidal disturbances. It possesses a generally rounded form, leaning slightly toward an intermediate shape rather than perfectly spherical or cigar-like. There may be subtle indications of a very minor disturbance. Overall, the galaxy's structure suggests a relatively quiescent system, potentially with limited current star formation within it.
