The galaxy appears as a moderately inclined disk galaxy. The central bulge presents a yellowish hue, possibly indicating an older stellar population. Moving outward from the core, there's evidence of a disk-like structure. A faint bluish tint is visible in parts of the outer disk, suggesting the presence of younger, hotter stars and ongoing star formation. There is a slight warp or irregularity in the shape of the disk, possibly hinting at past interactions or minor disturbances. There does not appear to be an actively merging galaxy nearby, but possibly an older interaction has slightly warped its morphology. The galaxy's overall structure seems mostly intact, with no large distortions or tidal tails visible in the image.
