The galaxy presents as a relatively compact and luminous object. Its overall morphology is largely smooth and elliptical, with a notable concentration of light towards the center. The core region exhibits a yellowish hue, suggesting an older stellar population with a lower rate of ongoing star formation. Fainter, bluer regions extend outwards from the core. There is some suggestion of minor disturbances in the galaxy's morphology. A small amount of internal structure may exist, but this is difficult to discern, indicating that the galaxy may be undergoing interactions or minor mergers.
