This galaxy presents as a disk-shaped system viewed nearly edge-on. A central bulge is discernible, exhibiting a slightly elongated and mildly boxy morphology. The disk component appears relatively smooth, with no immediately apparent spiral arm structure or prominent dust lanes visible in this observation. The color gradient suggests a radial distribution of stellar populations, with the bulge region exhibiting a redder hue. There's a hint of blue in the outer regions of the disk. There is no evidence of a ongoing major merger. There may be a very faint indication of tidal disturbances.
