This galaxy exhibits a somewhat irregular morphology. It appears to be composed of several distinct regions. The brightest and most concentrated region, located near the center, displays a yellowish hue, likely indicating an older stellar population. A second region is less bright and is redder in color. Diffuse spiral arms extend from the main body, but they are not well-defined, suggesting a lack of strong density waves. The spiral structure indicates a disk component. There may be an obscured bar structure present. The galaxy seems to have a moderate-sized bulge. Evidence of significant gravitational disturbance or interaction with another galaxy is visible, perhaps undergoing a merger.
