The galaxy presents as a relatively smooth, elliptical structure, exhibiting a central bulge that appears bright and somewhat concentrated. There's evidence of tidal disturbances, likely indicative of an ongoing or past merger event. A significant fraction of the galaxy’s light is emitted from a region with an effective radius of approximately 4 kpc. The overall color suggests a population dominated by older stars, resulting in relatively redder spectral properties. However, a small amount of blueish light, possibly due to new stars forming, suggests ongoing, albeit low, star formation activity. The estimated mass of the galaxy lies within the range of 10^10 to 10^11 solar masses. This is a relatively undisturbed system overall.
