The galaxy presents as a relatively small, faint, and elongated object. Its light is somewhat smooth and diffuse, with a slight concentration towards the center, indicative of a central bulge. The galaxy is likely an elliptical or lenticular type, viewed at an angle. There is an indication of disk-like features in the light distribution and the overall shape. The galaxy exhibits a subtle color gradient across its body, potentially signifying differing stellar populations or dust extinction. There is no clear evidence of strong star formation regions or spiral arm structures, suggesting a relatively passive system with little ongoing star formation.
