The galaxy presents as a fairly smooth, disk-like structure, viewed at an oblique angle relative to its rotational plane. There is a noticeable central bulge, appearing more concentrated and with a yellowish hue, possibly indicating an older stellar population. The disk component shows a subtle color gradient moving outward from the bulge, fading to a less saturated, slightly bluer color; although it is difficult to discern much variation in the disk. The overall morphology suggests it may be an early type disk galaxy, with the smooth appearance potentially arising from a lack of significant ongoing star formation in the disk, or a more dispersed spiral arm structure. The galaxy does not show any signs of major mergers or tidal disturbances in this image. The general shape appears to be somewhere between elliptical and a fully extended disk.
