This galaxy appears to be a relatively smooth, disk-shaped system, viewed at an oblique angle. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population. The disk component is less pronounced, and the colors become more muted, with a slightly bluer tint compared to the bulge. The overall morphology suggests a spiral galaxy, though the spiral arms are not clearly defined. The galaxy's profile is elongated and somewhat cigar-shaped, indicating a flattened structure. There is no apparent interaction or major disturbance, and the galaxy seems to be relatively isolated.
