The galaxy appears to be a disk galaxy, observed at an oblique angle relative to our line of sight. It exhibits a central bulge that appears relatively smooth and featureless, suggesting an older stellar population. The disk component of the galaxy displays some faint, diffuse spiral arm structure, though these arms are not well-defined. The overall color of the galaxy appears relatively uniform and moderately red, possibly indicative of a moderate rate of star formation. There is no clear evidence of a recent major merger or strong tidal interactions, but subtle distortions in the disk morphology might suggest minor disturbances or past interactions. The galaxy exhibits a small angular size, implying it's at a considerable distance.
