The galaxy appears as a somewhat elongated structure, exhibiting a dominant central bulge. The color gradient suggests a more pronounced concentration of older stellar populations towards the center, indicated by a reddish hue, with a transition to younger, bluer populations in the outer regions. The spiral arm structure, if present, is not clearly defined; the galaxy presents more of a disrupted or irregular morphology, possibly indicative of past or ongoing interaction or merger events. There is a slight asymmetry in the outer halo suggesting a tidal interaction or ongoing merging process, implying dynamical disturbance. There appears to be evidence of active or recent star formation occurring within the galaxy, particularly within the outer regions.
