The galaxy appears to be a relatively smooth, disk-like structure with a bright, concentrated central bulge. The overall shape is elongated, suggesting an elliptical or lenticular morphology, viewed at an angle. There's evidence of some bluer regions, perhaps indicative of star formation, particularly at the edges of the disk. While no obvious spiral arms are visible, the slight color variations and patchy distribution of light may hint at underlying structure. The central bulge exhibits a reddish hue, possibly due to older stellar populations, while the disk surrounding it transitions to a more bluish color profile. There may be some ongoing minor disturbance as suggested by the asymmetry, however no major interactions are visible.
