The galaxy presents as a somewhat elongated, disk-like structure, viewed at a significant angle. It exhibits a smooth, concentrated central bulge, which transitions into a fainter, more diffuse disk. The galaxy displays a yellowish-orange hue, indicative of an older stellar population. There's a subtle suggestion of internal structure within the disk, potentially hinting at spiral arm segments, though the resolution is insufficient to confirm. No obvious signs of significant recent star formation regions or dust lanes are apparent in this observation. There are no signs of interactions with other galaxies, suggesting it is currently undisturbed. The morphology is consistent with a relatively evolved galaxy, possibly of a lenticular type given the smooth appearance and angle.
