The galaxy presents a distinctly elongated, cigar-shaped morphology. It exhibits a relatively smooth appearance, with a possible disk-like structure viewed at a high inclination. The central region appears brighter and more concentrated, suggesting a bulge. The color gradient transitions from a yellowish-white core to a bluer outer region, potentially indicating ongoing or recent star formation in the outer disk, while the core contains an older stellar population. There is no evidence of strong tidal features or major disturbances, suggesting it is a relatively isolated system that may be experiencing minor interactions.
