The galaxy presents a somewhat irregular morphology. A central, concentrated region of higher luminosity exhibits a yellowish hue, potentially indicative of an older stellar population. Surrounding this central area, the galaxy displays fainter, bluer regions extending outwards. These areas suggest the presence of younger stars and potentially ongoing star formation activity. There appear to be some disturbances in the overall structure, with potential signs of tidal features or interactions. A more luminous region to the bottom right, with a similar colour as the galactic nucleus, could be indicative of a merger event or a region of intense star formation. The lack of a clearly defined spiral arm structure and the observed irregularities suggest the galaxy could be in a transitional stage, possibly evolving due to interactions with another galaxy or internal dynamic processes.
