The galaxy presents a flattened, disk-like morphology, likely a spiral galaxy seen at a moderately inclined angle. A central bulge is prominent, appearing rounded and exhibiting a yellowish hue, which suggests an older stellar population. Faint spiral arm structures are suggested, though not sharply defined due to the image's resolution. The arms show a bluer tint than the bulge, hinting at ongoing star formation within these regions. The disk appears somewhat disturbed, which may indicate some kind of interaction with another galaxy. There is a possible very small disturbance in the arm structure. The galaxy appears to be the dominant component of this system, showing no signs of a major merger.
