The galaxy exhibits a pronounced disk structure, viewed at a significant inclination relative to our line of sight. A bright, concentrated central bulge is observed, appearing smooth with a slightly elongated morphology. The disk shows evidence of some internal structure, potentially faint spiral arms or dust lanes, though the image resolution limits detailed assessment. The color distribution suggests a population gradient, with the central bulge appearing more red-shifted and the outer disk exhibiting a bluer hue, indicating younger stellar populations in the periphery. There is a hint of some minor tidal interaction or asymmetry, perhaps indicating a past or ongoing minor merger event, or other disturbance. 
