The galaxy appears to be a relatively large, disk-shaped system, oriented nearly edge-on with respect to our line of sight. A prominent central bulge dominates the galaxy's morphology. The bulge exhibits a smooth, yellowish-orange hue, suggesting an older stellar population. The disk is fainter than the bulge and shows a bluer tint. There is an indication of some features within the disk, but at this resolution, it's difficult to confirm distinct spiral arm structures. The galaxy displays a slight warp, possibly indicating a gravitational interaction or merger in its past. There is no visual evidence of recent or ongoing major merging activity. Overall, this galaxy appears to be a relatively quiescent system with a dominant bulge and a somewhat disturbed disk.
