The galaxy presents a generally elliptical morphology, appearing relatively smooth and centrally concentrated. The light distribution is somewhat diffuse. There is a clear central bulge, which is fairly luminous, surrounded by a less bright, more extended halo. The galaxy shows a noticeable reddish tint, which could suggest an older stellar population. There is a subtle indication of a disk structure with a slight elongation, though the overall structure is predominantly elliptical. There are no apparent signs of ongoing major merger activity or significant tidal disturbances, although there may be some minor irregularities in the outer regions. Overall, the galaxy gives the impression of a mature, relatively quiescent system.
