The galaxy presents as a spiral type, characterized by prominent spiral arms emanating from a central region. The spiral arms are loosely wound, showing a distinct open structure. Two main arms are clearly visible, exhibiting enhanced blueness, suggestive of ongoing star formation within these regions. A moderate bar structure appears to bisect the central bulge, potentially influencing the morphology of the spiral arms. The bulge itself is moderately sized relative to the overall disk. Evidence of potential minor interaction or disturbance is noted, with some asymmetry in the arm structure and light distribution. The overall color suggests a actively star forming system.
