The galaxy presents a somewhat elongated, cigar-shaped morphology. A central, bright region exhibits a bluer hue, possibly indicative of ongoing star formation. This is surrounded by a more diffuse, greenish halo. There may be some dust lanes or features obscuring the central region, lending to its non-uniform appearance. Overall, the galaxy appears relatively smooth, but not perfectly elliptical, suggesting some internal structure. It does not obviously appear to be undergoing a major merger, but minor disturbances or interactions may be present. The observed color gradient from blue in the core to green in the outer regions may indicate variations in stellar populations or dust content across the galaxy.
