The galaxy presents as a disk galaxy, viewed at an angle between face-on and edge-on. It exhibits a bright, concentrated central bulge that appears yellowish, suggesting an older stellar population. The disk shows a faint, bluish hue that possibly extends outwards and it gives the impression of ongoing star formation within the galaxy. The disk appears elongated, with a shape closer to cigar shaped than round, indicating a non-negligible inclination relative to the observer. A slight asymmetry can be seen, potentially indicating a minor disturbance in the galaxy's morphology. This could be due to a past or ongoing minor merger event.
