The galaxy appears as a moderately inclined disk galaxy with a prominent central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population with diminished recent star formation. The disk surrounding the bulge shows a bluer color gradient with increasing distance from the center, possibly indicating ongoing star formation in the spiral arms. While not sharply defined, there is a hint of spiral structure in the outer regions. The overall morphology indicates a relatively smooth appearance, but faint disturbances cannot be ruled out. There is no immediately obvious evidence of a major merger event but a minor interaction might be influencing the disk shape.
