The galaxy presents as a relatively compact, disk-shaped structure viewed at a high inclination. The central region exhibits a bright, concentrated core suggesting a significant stellar population and/or active galactic nucleus. The disk component shows a smooth texture overall, with little evidence of well-defined spiral arms. There appears to be subtle color variation within the disk, trending towards bluer hues in the outer regions. It's shape seems to suggest a minor merger event may have occurred, or that there is tidal debris. The system appears to be undergoing some form of interaction or disturbance, possibly with a smaller companion galaxy.
