The galaxy presents a discernible spiral structure with a prominent, moderately sized bulge at its center. The spiral arms are relatively tightly wound, tracing a path from the core outwards. While distinct, the arm structure is somewhat ill-defined, possibly due to distance and resolution constraints. The galaxy's central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the disk show a bluer tint, hinting at ongoing star formation. There may be a weak bar present at the center. The disk is oriented approximately face-on from our vantage point. There's no obvious evidence of a major merger event, however, a minor disturbance cannot be ruled out.