The galaxy presents a concentrated central bulge that emits strongly in the visible spectrum, appearing nearly spherical in shape. There are hints of a surrounding, more diffuse disk extending outward from the core. This outer region displays an irregular morphology. The galaxy appears to be a relatively mature system, with an indication of ongoing, albeit potentially low-level, star formation within its structure. The overall color indices suggest a population of both young and old stars. There are no strong signs of major recent merger events, although a subtle asymmetry in the outer disk may indicate a past interaction or minor disturbance. The galaxy exhibits a smooth, slightly elongated profile, with a relatively high Sersic index, indicative of a centrally concentrated light distribution.
