The galaxy presents a morphology that appears to be undergoing a possible interaction or merging event. There is a central concentration of light that suggests a core, or bulge component, with a generally smooth overall appearance, and there are potentially disturbed features surrounding this core. The color profile exhibits a variation, shifting from slightly bluer hues in some regions to redder tones in others. The luminosity indicates that, assuming the redshift is accurate, this is an intrinsically bright galaxy. The shape appears somewhat elongated.