The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a notable central bulge exhibiting a yellowish hue. Surrounding this bulge, a fainter, more diffuse region with a slightly bluish tint can be observed, suggesting the presence of a stellar disk or extended halo. There is a slight asymmetry in the outer regions, perhaps indicating minor tidal disturbances. However, there is no clear evidence of a major merger event or strong spiral arm structures. Overall, the galaxy appears to be relatively quiescent in its present state.
