The galaxy presents as a spiral galaxy, seen at a slight angle to our line of sight. The central bulge appears prominent, but not overly dominant, displaying a smooth, concentrated luminosity. The spiral arms are well-defined, emanating from the core region. The galaxy exhibits a two-armed spiral structure. The spiral arms are moderately wound and have a granular texture, suggesting the presence of numerous star-forming regions. There is a slight asymmetry in the distribution of light and matter, potentially indicating a minor gravitational interaction or disturbance. The overall color profile suggests a mix of stellar populations, with bluer hues observed in the spiral arms implying ongoing star formation and redder tones in the central bulge, indicating older stellar populations. There is no obvious presence of a strong bar structure.
