The galaxy presents as a largely smooth, centrally concentrated object. Its overall form approximates a spheroid with a high degree of roundness. There is minimal indication of disk-like features or spiral arms. The galaxy exhibits a radial gradient in surface brightness, with a bright, compact core gradually fading into a more diffuse halo. Color gradients suggest a higher concentration of older stellar populations within the central regions. The morphological classification indicates that the galaxy is unlikely to be undergoing a major merger event and does not exhibit strong tidal features or disturbances, but does show some level of disturbance. Weak signs of star formation might be present, but are not especially notable. The object could be consistent with an elliptical galaxy at an estimated distance, although the possibility of a highly inclined spiral galaxy cannot be completely ruled out with the available data.
