The galaxy appears as a generally smooth, somewhat elongated structure. The light distribution suggests a higher concentration of stars towards the center, with the surface brightness gradually decreasing towards the outer regions. The galaxy's morphology leans more towards an elliptical type, but it could also be a spiral galaxy seen at an angle. There might be a hint of a faint disk, but the smooth and dominant central bulge makes it difficult to confirm spiral arm features. There are no obvious signs of intense recent star formation, which aligns with the smooth appearance. The galaxy is not perfectly round, and there is a slight elongation, but not a cigar shape. The galaxy does not show obvious signs of major disturbances or merger activity, but possible minor disturbance.
