The galaxy presents as a spiral galaxy with a notable central bulge. The bulge appears bright and moderately sized relative to the overall galactic disk. The spiral arms are tightly wound and somewhat indistinct, with a bluish hue suggesting active star formation. The galaxy exhibits a high degree of flattening, with a ratio of minor to major axis of approximately 0.5, indicating a significant inclination to our line of sight. There is no strong evidence of a bar structure, and while the arms are tightly wound, there is little to no signs of any major disturbances or interaction with another galaxy. The colour profile suggests that the outer regions are actively forming new stars, while the bulge is likely composed of older, redder stellar populations.
