The galaxy presents a complex morphology, exhibiting characteristics of a system undergoing a merger or interaction. The primary body of the galaxy appears somewhat amorphous, with a central region that is relatively smooth and concentrated. A tidal feature or arm-like structure extends from one side of the main body, showing a distinct, possibly disrupted, area of star formation, indicated by a bluish tint. There is a notable companion galaxy, or a region of intense star formation within the main galaxy, that appears as a slightly blurred, elongated structure. This region is connected to the main body, implying gravitational interaction. Evidence suggests the possibility of ongoing tidal interactions, as the overall shape deviates significantly from a regular elliptical or spiral form. There seems to be a small central bulge. The color profile indicates a mix of stellar populations, with both older, redder components and younger, bluer regions present.
