The galaxy presents as a largely smooth, centrally concentrated object. It has a broadly elliptical morphology with a hint of a more circular, rounded appearance. The central region exhibits a bright, yellowish-white core that suggests an older stellar population. A subtle color gradient is present, with the outer regions exhibiting a slightly bluer hue compared to the central core. This suggests the potential presence of younger stars in these peripheral areas, though their contribution seems relatively limited. There's no clear indication of spiral arms or prominent dust lanes. Faint wisps or features may be present in the immediate vicinity, but it is difficult to determine their origin.
