This galaxy appears as a diffuse, elliptical-shaped object with a smooth, homogenous texture. The color profile is primarily reddish-yellow, suggesting a population of older stars and a low rate of ongoing star formation. The object's light is centrally concentrated, with luminosity decreasing towards the outer edges. The galaxy presents a high degree of rotational symmetry. There is potentially a minor disturbance nearby or some minor signs of a merger or tidal interaction, though the galaxy maintains a relatively undisturbed structure. The morphological properties of the observed system show signs of older stellar populations.

