The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge is apparent, exhibiting a bright, whitish-yellow hue. The luminosity gradually decreases moving outwards from the core, with an extended halo that appears more diffuse and slightly bluer. No distinct spiral arms or bar structures are discernible. There might be a minor asymmetry to the galaxy's overall shape, but it appears mostly relaxed and undisturbed. The color gradient suggests an older stellar population dominates the bulge, with potential pockets of more recent star formation in the outer regions.
