The galaxy presents as a largely smooth, elliptical-like structure, with a high degree of central concentration. There is little evidence of spiral arms or significant disk features. Color gradients appear subtle, exhibiting a slightly redder hue towards the central region, suggesting a potential older stellar population concentrated toward the core. A faint, diffuse, greenish-yellowish halo surrounds the central region, fading into the background. There are no visually apparent signs of ongoing major merger activity or significant tidal disturbances, though the possibility of minor disturbances cannot be ruled out due to the limited resolution. The galaxy presents a relatively undisturbed, relaxed morphology.
