The galaxy presents as a distorted spiral or possibly an elliptical galaxy with a slight elongation. The light profile appears relatively smooth, with a central concentration that suggests a bulge component. There is a suggestion of a disk but with disturbed arms or tidal features. A portion of the galaxy exhibits a bluer color, potentially indicating younger stellar populations and ongoing star formation. Other regions are redder, suggesting older stars or dust obscuration. Overall, the morphology is somewhat irregular, possibly the result of an interaction or merger. The luminosity is significant, indicative of a substantial stellar mass.
