The galaxy appears to be an elongated, disk-shaped system, likely viewed at a high inclination angle. The central bulge is moderately prominent, displaying a yellowish hue, suggesting an older stellar population. The outer regions exhibit a bluer color, possibly indicating ongoing or recent star formation within the disk. The galaxy's overall form is relatively smooth, with no readily apparent spiral arm structure or major disturbances detected in the image. The light distribution tapers off gradually from the center to the edges, suggesting a well-mixed stellar population. The estimated size is a few kiloparsecs across. There is a potential companion object present very far away from this system. The galaxy does not appear to be undergoing a major merger, although there might be some minor tidal features or a faint plume.
