This galaxy presents a distinctly elongated, cigar-shaped morphology. There appears to be a smooth, centrally concentrated bulge region exhibiting a yellowish-orange hue. Extending outward from this central region are fainter, bluer, and more diffuse components. The overall structure suggests a disk-like component viewed at a high inclination angle. No obvious spiral arm structures are visible, and there is no strong evidence of tidal features or major disturbances indicative of an ongoing or recent merger event. The light distribution implies that the stellar population in the center may be older, while the outer regions exhibit bluer colors, possibly indicating more recent star formation. The galaxy shows minimal signs of ongoing galactic interaction.
