The galaxy presents a flattened, elliptical morphology. Its central region exhibits a bright, concentrated luminosity, appearing yellowish-orange in color, suggesting an older stellar population dominating the core. The disk, extending outwards from the core, demonstrates a bluer hue. This color gradient from core to disk suggests ongoing or recent star formation in the outer regions. The galaxy appears relatively smooth in texture, lacking prominent spiral arm structures or intense star-forming knots. A subtle distortion or extension is visible, indicating a potential minor gravitational interaction or tidal feature. The overall shape is elongated, classified as cigar-shaped, rather than perfectly round. There are no signs of a major ongoing merger.
