The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge exhibiting a yellow-orange hue. This suggests a population of older stars. There's minimal evidence of spiral arms or a distinct disk. The light distribution appears fairly concentrated, indicating a high degree of sphericity.  There is a smaller, dimmer secondary object in the field of view. Based on the tidal features there appears to be some disturbances occurring as it seems to be in the beginning stages of merging.

Given its luminosity and overall morphology, this galaxy is likely a massive, quiescent system, possibly residing on the red sequence. The apparent color suggests a relatively low rate of ongoing star formation.
