The galaxy appears to be a disk galaxy, observed nearly edge-on from our line of sight. There is a distinct central bulge that exhibits a yellowish hue, suggesting an older stellar population. The disk component of the galaxy presents as a flattened structure extending from the bulge. The disk also appears to be somewhat amorphous and exhibits a bluer color than the bulge, potentially indicating the presence of ongoing star formation regions within the disk. There is very slight indication of internal structure, but overall the galaxy appears smooth. There is no visual evidence of a major merger event, however, there is slight asymmetry to the disk, suggesting a minor gravitational disturbance.
