The galaxy presents as having an overall elliptical morphology, though exhibiting some irregularities. The light distribution is concentrated towards the center, indicating a central bulge, with a smoother, more diffuse halo extending outwards. The color gradient shifts from a reddish hue towards the core to a bluer tint in the outer regions. This could indicate older stellar populations in the center and younger, hotter stars in the periphery. There appear to be some asymmetric features suggesting possible minor tidal disturbances or interactions. There are subtle indications of a disk, but it is not clearly defined. There is also a small knot or region of intense red color.
