This galaxy exhibits a morphology that appears to be undergoing a disturbance. The core is characterized by a bright, relatively smooth and concentrated region, possibly indicating a spheroidal component or bulge. Extending from this central area is a fainter, elongated feature. This extended structure displays a gradient in color, shifting from a reddish hue near the central region to a bluer tint further away. The irregular shape of this feature suggests a possible tidal tail or stream resulting from a gravitational interaction or merger event. Overall, the galaxy's light distribution is not symmetrical, and it demonstrates a disturbed morphology. There appears to be a hint of a possible disk or arm structure distorted by an ongoing interaction.
