The galaxy presents as a generally smooth, centrally concentrated object. The core exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the central region is a more diffuse bluish halo, potentially indicating the presence of younger, hotter stars or ongoing star formation, although the smoothness suggests a more gradual and less intense process. The overall shape appears close to round, lacking any obvious spiral arm structures or a pronounced disk. There is a slight asymmetry or minor perturbation visible in the outer regions, hinting at a possible past interaction or disturbance but the galaxy appears relatively undisturbed. The size is moderate, and there is no apparent active galactic nucleus. The estimated mass is likely in the range of a typical galaxy. Star formation appears to be present but not dominating the appearance of the galaxy.
