The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The luminosity profile appears to be centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The galaxy appears to be somewhat lenticular in shape, being more "in between" elliptical and disk-shaped. Hints of a faint, diffuse disk are subtle and may be an artifact.

There appears to be a faint blueish halo surrounding the central region.

Overall, based on its morphology, this galaxy appears to be a reasonably massive system, likely nearing the end of its star forming processes, with a significant fraction of its stellar population being older. There might be weak ongoing star formation indicated by the bluer hue. Finally, there are subtle but present minor disturbances, hinting at a potential interaction with a satellite galaxy.
