The galaxy presents as a largely smooth, centrally concentrated object with an elongated, ellipsoidal morphology. The core region displays a yellowish hue, possibly indicating an older stellar population. Moving outward from the center, the light gradually fades into a diffuse, bluish halo. There is a subtle hint of asymmetry along the galaxy's edges, potentially suggesting minor tidal interactions or disturbances, though no clear signs of a major ongoing merger are evident. Overall, the galaxy's smooth appearance is consistent with an early-type galaxy, such as an elliptical or lenticular. The lack of any prominent spiral arm structures or concentrated knots of star formation further supports this classification.
