The galaxy exhibits a disk-like structure, but the presence of a prominent bulge suggests a possible classification as an intermediate spiral or lenticular galaxy. The central region appears smooth and concentrated, indicating a high stellar density. The disk shows hints of spiral arms, although they are not well-defined or tightly wound. There is some color variation within the disk. A small, bright blue region located towards the bottom of the galaxy likely indicates an area of active star formation. There is the possibility of a minor interaction given some asymmetries in the disk.
