The galaxy exhibits a somewhat flattened, elliptical morphology, with an apparent disk-like structure viewed at an angle. There's a noticeable central bulge, which appears to be a more concentrated, brighter region, potentially indicating a higher density of older stellar populations. Extending outward from the bulge, a fainter, bluer disk component is observed, suggesting the presence of younger stars and ongoing star formation. The blue tint is indicative of the presence of hot, young stars. The disk appears somewhat disturbed or irregular, possibly due to past interactions or internal dynamics. The overall structure suggests a galaxy that may be transitioning between a more elliptical and a spiral morphology, or perhaps an elliptical galaxy undergoing some star formation in its outer regions.
