This galaxy presents a morphology that is largely smooth and elliptical in appearance, but with some evidence of possible tidal interactions. It exhibits a centrally concentrated luminosity profile, with the highest intensity core appearing golden in color, indicative of an older stellar population.

Extending outwards from the bright core, a fainter, more diffuse halo is observed. There is a slight elongation or asymmetry to the halo, hinting at possible gravitational interactions with a nearby companion object.

The color gradient within the galaxy appears to shift from the golden core to slightly bluer hues in the outer regions of the halo, suggesting the presence of younger stars in those areas, but overall the blue star formation activity is low.

There is also a second object or merging galaxy with high star formation activity, as indicated by its very blue hue.

Overall, this system seems to be in a relatively advanced stage of evolution, potentially either just having experienced, or currently undergoing, a merger or interaction with the other galaxy.
