The galaxy presents as a relatively face-on spiral galaxy with a prominent, moderately sized bulge. Spiral arms are clearly visible, exhibiting a defined, two-armed structure with an intermediate winding pattern. The arms appear somewhat patchy, suggesting areas of active star formation. A strong bar structure appears to be present, bisecting the central bulge. There is no evidence of significant ongoing mergers or major disturbances. The overall color suggests a mix of older stellar populations in the bulge and younger, bluer stars in the spiral arms, indicating ongoing star formation within the disk.