The galaxy presents as a spiral type, with a moderately sized central bulge exhibiting a yellowish hue, suggesting an older stellar population. Two prominent spiral arms extend from the central region. These arms display a relatively well-defined, yet somewhat patchy structure, indicating ongoing, but perhaps not exceptionally vigorous, star formation. The arms appear to wind moderately tightly around the bulge. A strong bar-like structure is observed traversing the bulge region, likely influencing the morphology of the spiral arms. The overall color profile suggests a mix of stellar populations, with younger, bluer stars concentrated in the arms and older, redder stars dominating the bulge. There are no obvious signs of a major merger event, although a slight asymmetry in the arm structure could indicate a minor gravitational interaction or internal disturbance.
