The galaxy exhibits a distinct spiral structure, characterized by two prominent arms that emanate from a central bulge. The spiral arms are moderately wound, displaying both medium and loose morphologies. Star formation appears active within these arms, evidenced by the presence of bluer regions. The central bulge exhibits a less prominent yellowish hue, suggesting an older stellar population compared to the arms. The bulge size is moderate to small relative to the overall disk of the galaxy. There is no apparent strong bar structure bisecting the bulge, although a weak bar may be present. The galaxy's disk is not viewed edge-on, but rather at a shallow angle, allowing for clear observation of the spiral arm structure. There are hints of minor disturbances in the galactic structure, but the overall morphology suggests no ongoing major merging events.
