The galaxy presents a somewhat disturbed morphology. A significant portion of the galaxy appears disk-like, yet lacks a clear spiral arm structure. The disk exhibits an off-center bulge component with a yellowish hue, suggesting a relatively older stellar population. Diffuse blue regions are observed, indicative of ongoing or recent star formation, particularly in the areas surrounding the central bulge. 

There appears to be evidence of a possible interaction or merger event influencing the galaxy's structure, with faint tidal features or distortions visible. These include diffuse extensions of material emanating from the main galactic body. The overall colour suggests an actively evolving system with a mix of stellar populations.
