The galaxy presents a spiral morphology, viewed at a near face-on orientation. Two prominent spiral arms are discernible, exhibiting a moderate degree of winding. The central bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy. The color distribution indicates a mix of stellar populations, with a yellowish hue dominating the bulge region, suggesting older stars, and bluer tones evident in the spiral arms, implying ongoing star formation. There is no clear indication of a strong bar structure bisecting the galaxy. The overall structure appears relatively undisturbed, with no obvious signs of major recent merger events.
