The galaxy exhibits a disturbed morphology, likely indicative of an ongoing or recent interaction. The primary component presents as a moderately bright, somewhat elongated spheroid. It appears to possess a relatively smooth luminosity profile, with a central concentration. There is evidence of tidal features, extending in a plume-like structure from the main body. This plume displays a gradient in color, transitioning from reddish hues closer to the core to a more diffuse, yellowish tint distally. There seems to be a secondary object near one end of the spheroid, bluish in color. The is indicative of significant star formation. The general color profile suggests a moderate redshift. Overall, the system shows signs of dynamical instability and active star formation associated with an interaction event.
