This galaxy presents as a system undergoing a significant merger event. The morphology is heavily disturbed, with visible tidal features indicative of strong gravitational interactions. A primary central bulge is readily apparent, exhibiting a yellowish-white color, suggesting a population of older stars. This bulge is surrounded by a fainter, more diffuse halo.

There is a secondary, smaller condensation of light, possibly the core of the merging galaxy, located to the side of the main bulge. The color of this secondary component also indicates an older stellar population, with a similar yellowish hue. Between the two components is a region of enhanced star formation, traced by blue light. This may have been triggered by the ongoing interaction. 

Overall, the galaxy is actively evolving, with morphology shaped by a merger of two galaxies of substantial mass. The ongoing interaction is inducing new stellar formation, resulting in a complex, dynamic system.
