This galaxy presents as a spiral or disk-like structure. Its disk shows a noticeable tilt, allowing a partial view of the galactic plane. The central bulge appears bright and concentrated, with a yellowish-white hue, suggesting an older stellar population. Extending outward from the bulge is a fainter, bluer disk. The disk contains some irregularities, which may be spiral arm segments, but the image resolution limits certainty. Star formation may be present within the disk. No clear signs of major mergers or tidal disturbances are visible in the immediate vicinity, suggesting that the galaxy's present morphology is largely undisturbed.
