The galaxy presents a moderately concentrated morphology, exhibiting a somewhat irregular structure. There is evidence of interaction or disturbance, potentially indicating an ongoing or recent merger event. The galaxy appears to have a relatively smooth central region, transitioning into fainter, more diffuse outer regions. It is moderately luminous in the observed bands, with a color profile suggesting a mixture of stellar populations. The apparent size indicates that this is a moderately sized galaxy for its redshift. The asymmetry in the outer structures hints at possible tidal features or debris from the interaction.
