The galaxy appears to be a spiral galaxy, inclined relative to our line of sight. It displays a bright, concentrated central bulge that fades smoothly outward. The disk component shows evidence of spiral arm structure. The colour profile shifts from yellow-white near the center to bluer hues in the outer regions of the disk. Dust lanes appear to be present within the spiral arms, contributing to a mottled texture. The overall morphology suggests a system that is relatively undisturbed, without strong signs of recent major merger activity. There is a faint, extended halo.
