The galaxy presents an elliptical morphology with a dominant, smoothly distributed light profile. There is a bright, unresolved core region exhibiting a greenish hue, indicating elevated emission in shorter wavelengths. A fainter, extended halo of less defined structure is visible, showing a reddish-white color, which suggests a relatively older stellar population. The galaxy exhibits a lack of spiral arms or a prominent disk structure. There is a hint of disturbance or asymmetry, suggesting potential past or ongoing interaction with another celestial body. Overall, the galaxy appears to be relatively compact and quiescent.
