The galaxy appears to be a lenticular or early-type spiral galaxy, seen at an oblique angle. The central bulge exhibits a smooth, bright, and concentrated luminosity profile, appearing yellowish-white. The disk component is less prominent, showing a bluer hue suggesting the presence of some younger stars or star-forming regions, albeit subdued. There is a slight indication of spiral arm structure, though it is faint and tightly wound. The galaxy appears elongated, with a cigar-like shape, lacking significant irregularities or prominent tidal features, which suggests it is in a relatively relaxed state with no major recent mergers. There is a notable difference in colour between the bulge and the outer regions of the disk. The galaxy appears to be a massive system with a moderate rate of star formation.
