The galaxy appears to be an interacting system, consisting of two distinct galactic bodies. Both exhibit an elliptical morphology, with one appearing significantly more elongated than the other. The brighter, more elongated galaxy shows evidence of a concentrated central bulge with a smooth luminosity gradient outward. The less elongated, companion galaxy, is positioned nearby, and appears to be influencing the overall structure of the brighter galaxy. There is no evidence of spiral arm structure in either of the galaxies. The color is indicative of older stellar populations, with a higher concentration of light in the redder wavelengths. The interaction between these two bodies suggests a system undergoing a process of gravitational merging.
