The galaxy presents as a flattened, elliptical structure, likely a disk galaxy viewed at an oblique angle. A central bulge is visible, exhibiting a yellowish-white hue, indicative of an older stellar population. The disk component appears less defined, showing a mottled bluish-white coloration that suggests the presence of younger, hotter stars and ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There might be minor asymmetry within the disk; however, further investigation is needed to confirm the presence of any faint tidal features or minor disturbances.
