The galaxy presents a disturbed morphology, potentially indicative of an ongoing or recent interaction. Its light profile exhibits a deviation from a smooth elliptical shape. There appears to be a central bulge surrounded by diffuse light. The morphology suggests it has a possible tidal tail or bridge feature, extending to the lower left. The color profile shows a mixture of colors, the redder bulge light is more pronounced. Blue colors might be the result of active star formation regions, possibly triggered by the interaction. Although the galaxy is not extremely bright, it is quite large, and with a likely stellar mass of above 10^10 solar masses, we can assume this galaxy to be pretty massive.
