The galaxy presents as a centrally concentrated system with a smooth light distribution. The core exhibits a yellowish hue, possibly indicative of an older stellar population. Surrounding the core, a more diffuse, bluish halo extends outward, suggesting the presence of younger stars. The overall shape appears elliptical, with a minor elongation along a particular axis. There is no evidence of prominent spiral arms or significant dust lanes. The galaxy displays a relatively high degree of symmetry and appears largely undisturbed, lacking any obvious signs of recent merger activity. The color gradient from the core to the outer regions suggests a radial variation in stellar populations.