The galaxy presents as a barred spiral with a relatively high degree of inclination relative to our line of sight. The central bulge appears prominent and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. Spiral arms are faintly visible, displaying a mottled texture with subtle variations in color. There appears to be some minor morphological disturbance within the disk, but it is unclear if this is from a merging event or is a local fluctuation within the arm structure. The overall color profile suggests a galaxy with moderate levels of ongoing star formation, though potentially lower when averaged across the entire galaxy. The elongated appearance confirms a disk-like structure, with the primary axis extending approximately 7 arcseconds. The galaxy is not perfectly smooth, as some substructures can be seen.
