The galaxy presents as a moderately bright, elliptical-like structure. The light distribution appears relatively smooth, with a concentration towards the center, suggesting a prominent bulge. There is a noticeable color gradient, shifting from a yellowish hue in the core to a slightly bluer tint in the outer regions. No obvious spiral arm structures or dust lanes are visible. The galaxy appears largely undisturbed, showing no signs of ongoing major merger activity, although subtle disturbances cannot be ruled out. The overall morphology points towards a galaxy with an older stellar population in the central regions and possibly ongoing, but low, star formation activity in the outskirts.
