The galaxy appears to be a disk galaxy, exhibiting a roughly elliptical shape. The central region displays a concentrated, brighter core, possibly indicative of a bulge component. Surrounding the core, fainter, more diffuse light suggests the presence of a disk. The color gradient shifts from a yellowish-orange hue in the center to a greenish-blue periphery, potentially revealing differing stellar populations or dust content. The overall morphology suggests the galaxy is experiencing some minor disturbances in its structure.
