The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a bright, well-defined core. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, subtly transitioning to a redder tint in the outer regions. There is no discernible spiral arm structure or prominent dust lanes. The overall shape is largely circular, with minimal elongation or distortion, indicating a relaxed and potentially evolved system. There is only the slightest evidence of disturbance.
