The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a generally smooth morphology, with minimal discernible features such as spiral arms or dust lanes. The light distribution appears relatively uniform, suggesting an older stellar population. The core appears quite concentrated, exhibiting an intense yellow color. A faint halo surrounds the central region, fading gradually into the background. The overall shape seems approximately circular, with only a slight deviation from perfect roundness. There is no visually apparent evidence of ongoing major mergers or tidal disturbances, although minor disturbances are not ruled out at this resolution.
