The galaxy presents as a relatively bright, disk-shaped structure seen at an almost edge-on orientation with a slight tilt. A central bulge region, approximately 1/3 the diameter of the disk, is visible and appears slightly brighter and yellower than the surrounding disk, indicating an older stellar population. The disk itself shows some evidence of spiral structure, primarily visible as subtle variations in color and brightness along the disk's length. The outer regions of the disk appear somewhat fainter and bluer than the inner regions. The overall color suggests a mixed stellar population with both older, redder stars in the bulge and younger, bluer stars in the disk. The galaxy does not show any significant signs of ongoing major merger activity, although there is a slight irregularity in the disk shape indicating minor interaction. The galaxy's smooth appearance and the color distribution are consistent with an intermediate-mass galaxy with a moderate star formation rate.
