The galaxy presents as a disk-shaped system with an elliptical morphology. The central bulge appears luminous and exhibits a color gradient transitioning from a warmer yellow-orange hue in the innermost regions to a cooler green-yellow towards the outer edges. The disk component appears relatively smooth, suggesting a lack of prominent spiral arm structures, though faint blueish-green hues on the galaxy's periphery may indicate regions of star formation. The overall structure suggests a system in an intermediate evolutionary state, not fully spheroidal but exhibiting significant bulge prominence. The galaxy shows a moderate degree of ellipticity, appearing somewhat elongated, but not highly distorted. There is no obvious evidence of ongoing major merger activity or strong tidal disruption in the immediate vicinity.
