This galaxy appears to be an elliptical galaxy, presenting a largely smooth and symmetrical morphology. The galaxy's light distribution is concentrated towards the center, exhibiting a bright, well-defined nucleus. Moving outwards from the core, the light gradually fades into a more diffuse halo. There's a noticeable lack of distinct spiral arms or prominent dust lanes, which supports its classification as an elliptical galaxy. The overall color is somewhat uniform, suggesting an older stellar population with minimal ongoing star formation. There might be a hint of slight perturbation in the outer regions, but overall it looks like a fairly relaxed system, likely not undergoing any major merging events currently.
