The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. The core region is significantly brighter, appearing almost as a single unresolved point of light. The galaxy exhibits a fairly regular, rounded morphology with little to no evidence of spiral arms or a prominent disk. There is no visible dust lane obscuring the central region. There is an absence of major tidal features or morphological irregularities suggestive of recent or ongoing mergers. The galaxy appears to be a relatively isolated system, not clearly interacting with any other nearby galaxies in the field of view. A faint halo appears to extend beyond the main body of the galaxy. The overall color suggests an older stellar population, with a bias towards redder wavelengths and a lower rate of star formation.
