The galaxy presents as a relatively smooth, lenticular or early-type spiral system, exhibiting a predominantly elliptical morphology. It is observed nearly edge-on. The central bulge is prominent, displaying a concentrated luminosity profile. The surrounding disk appears moderately flattened, showing some hints of spiral structure, though these are not sharply defined. Color gradients suggest that the central region may have a higher concentration of older stellar populations, indicated by its yellowish hue, whereas bluer colors are less apparent in the disk. There's no clear evidence of ongoing major star formation, and any spiral arms or features present are faint and tightly wound. There are no obvious signs of recent merger activity or significant tidal disturbances. The galaxy's overall structure indicates a system that has largely ceased active star formation, with a substantial fraction of its stellar mass contained within its bulge component.
