The galaxy presents a complex morphological structure. The light distribution suggests a galaxy in the process of merging or experiencing significant tidal interactions. A dominant, central bulge exhibits a smooth, but not perfectly circular, profile. Indications of ongoing or recent star formation are present within the system, primarily concentrated in what appear to be disturbed disk components or tidal features. These regions show a bluer color, suggesting the presence of younger, hotter stars. A significant portion of the galaxy exhibits redder colors, particularly in the central region, which could indicate an older stellar population. The overall appearance suggests a system that is not fully relaxed, with disturbed morphology likely indicative of ongoing dynamical processes. Faint, extended features hint at tidal tails or other remnants of past interactions.
