The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge which graduates smoothly outward into a less dense halo. The core of the galaxy shows a yellowish hue, potentially indicative of an older stellar population dominating this region. As the light diffuses outwards, it takes on a slightly bluer shift. There is no strong evidence of spiral arm structure or significant dust lanes. There appears to be a slight tidal disruption, but it is relatively smooth compared to the core. This would likely indicate a low star formation rate for a galaxy of this magnitude. The overall appearance suggests a system that has undergone significant evolutionary processes, leading to its current spheroid-like morphology.
