The galaxy presents as a fairly elliptical structure, with a smooth and relatively featureless morphology. The central region exhibits a concentration of light, appearing brighter and yellower than the surrounding areas. Moving outward from the core, the light gradually diminishes, transitioning into a more diffuse bluish halo. While there is some indication of asymmetry in the halo's light distribution, it is difficult to definitively characterize it as indicative of any specific structural feature like spiral arms, likely due to image resolution and/or galaxy type. Overall, the galaxy appears relatively undisturbed. The galaxy is more luminous in the redder bands than the blue ones, suggesting older stars comprise the majority of the observed stellar population. Based on the galaxy's relatively featureless appearance, it could be a lenticular galaxy, although the exact classification remains ambiguous.
