The galaxy presents as a disk galaxy, viewed at an oblique angle, nearly edge-on. It exhibits a bright, yellowish bulge component surrounded by a fainter, somewhat elongated disk. There is evidence of some patchy structure within the disk, possibly indicating spiral arm segments or dust lanes, but the resolution is insufficient to discern clear spiral arms. The color distribution suggests the presence of both older stellar populations in the bulge and some younger, bluer stars within the disk.  There is also a bright red area in the galaxy disk suggesting a potential region of star formation or active galactic nuclei. It appears relatively undisturbed, with no major signs of recent merger activity, although some minor irregularities or distortions cannot be ruled out at this resolution.
