The galaxy exhibits an irregular morphology, suggesting a system undergoing gravitational interaction or a recent merger event. A significant portion of the galactic light emanates from a central, concentrated region which displays a yellowish color. This could be indicative of an older stellar population or a region of intense star formation obscured by dust. Fainter, extended features appear to stretch outwards from this central region, showing a bluish hue, especially prominently in the Northern area, suggestive of more active, recent star formation associated with younger, hotter stars. These features are not symmetrically distributed, indicating disturbances to the overall structure. A tidal tail like feature seems to stem from the galaxy in the upper portion of the image. There is no clear evidence of a well-defined spiral arm structure or a prominent disk.
