The galaxy presents as a relatively smooth and centrally concentrated object. Its morphology appears to be largely spheroidal, possibly elliptical, with a high degree of symmetry. The light distribution exhibits a gradual decline in surface brightness from the core outwards. The core is bright, surrounded by fainter regions, with no well-defined spiral arms or other distinct features visible.

In terms of color, the galaxy appears to exhibit a slightly yellowish-white core, which hints at an older stellar population. The outer regions of the galaxy tend to be more bluish, which suggests the presence of a younger, star-forming stellar population. The galaxy may show some minor disturbances; however, the features of this are difficult to determine due to the distance.