The galaxy presents a distinct spiral morphology. The spiral arms are well-defined, exhibiting a relatively tight winding pattern as they emanate from the galactic center. Two prominent spiral arms are visible, displaying a relatively smooth texture with discernible substructure indicative of star-forming regions along their lengths. The central bulge appears moderate in size and exhibits a yellowish hue, suggesting an older stellar population within. No significant bar structure is apparent within the central region. There is no sign of any major merging events. The overall color suggests a presence of both young and old stars, implying ongoing star formation. The galaxy disk appears to be oriented closer to face-on, offering a relatively unobscured view of its structure.
