The galaxy presents as a spiral type, observed at a slight angle to our line of sight. It exhibits a well-defined, moderately sized central bulge, surrounded by a disk. Distinct spiral arms are visible, tightly wound around the central bulge. The arms appear to be relatively symmetrical, though the resolution is not sufficient to definitively ascertain the arm count. The color profile suggests ongoing star formation, with bluer hues present within the spiral arms. No major disturbances or tidal features are readily apparent, although a possibility of a minor interaction cannot be excluded based on this image alone. There is no visible strong central bar.
