The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. There's a smooth transition from this bulge into a less defined disk component. The disk is not observed edge-on; it appears closer to face-on with subtle spiral arms. Some asymmetry can be observed in the outer regions. The galaxy exhibits a color gradient, transitioning from a yellowish-white core indicative of older stellar populations to a bluer hue in the outer disk, suggesting ongoing or recent star formation. The galaxy appears relatively isolated with only minor signs of interaction or disturbance from nearby companions.
