This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger event. The overall shape is irregular, deviating significantly from a smooth elliptical or well-defined spiral structure. There's a suggestion of tidal features, possibly faint streams or plumes extending outward from the main body of the galaxy, though these are subtle. A brighter, somewhat amorphous region is apparent on one side, possibly indicating enhanced star formation triggered by the interaction. The galaxy exhibits a blueish hue, implying the presence of younger, hotter stars; this bluer region supports the assertion of recent star formation activity. The galaxy appears moderately compact. The luminosity is moderate, neither exceptionally bright nor particularly faint, within the context of similar galaxies at comparable distances.
