The galaxy appears to be undergoing a significant merger event. There is evidence of tidal disruption and interaction, with asymmetries present in the light distribution. The central region exhibits a somewhat amorphous structure, lacking a well-defined nucleus, suggesting substantial gravitational disturbance. Faint tidal tails or plumes may be extending outwards, further supporting the merger scenario. The color profile indicates a mixture of stellar populations, with bluer regions interspersed with areas of redder hues, potentially indicative of ongoing or recent star formation alongside older stellar populations. The overall morphology is irregular and disturbed, deviating significantly from a typical spiral or elliptical galaxy. The galaxy displays a moderate level of star formation activity, indicated by its intermediate color, but does not appear to be undergoing a major starburst. Its mass is estimated to be relatively low.
