This galaxy exhibits a complex morphology, appearing as a disturbed system potentially undergoing a merger or tidal interaction. There appears to be two main components, a somewhat smooth and diffuse central region that transitions into a more disturbed disk-like feature.

The central region exhibits a smoother texture with a slightly bluer hue, possibly indicating a population of younger stars. This region could be a remnant of an older elliptical galaxy, or the core of a spiral galaxy. The disk component shows evidence of significant disruption, with irregular patches of light and dark, possibly indicating recent or ongoing star formation. The color of this disk is reddish/yellowish.

Based on the overall morphology, it's likely this system is evolving dynamically, potentially through the accretion of a smaller galaxy or a close interaction with another system. Further spectroscopic analysis would be beneficial to determine the age and composition of the stellar populations in each component, and to confirm the presence of any tidal features not apparent in this image.
