This galaxy exhibits a pronounced elongated, cigar-like morphology. The central region displays a smooth, concentrated luminosity, potentially indicative of an older stellar population and possibly a supermassive black hole at its core. Extending outwards from the core are fainter, diffuse structures showing some evidence of disk-like features. Patches of bluer emission are observed in these outer regions, suggesting ongoing or recent star formation. The overall structure appears relatively undisturbed, with no strong signs of a recent major merger event. However, there are faint indications of minor disturbances or tidal features within the galaxy's outer regions, hinting at possible past interactions. The galaxy appears to be a spiral, viewed at high inclination.
