The galaxy presents as a lenticular or early-type spiral system. It appears highly elongated with a distinct cigar-shaped morphology. A prominent central bulge exhibits a smooth texture with a characteristic yellowish-orange hue, suggesting an older stellar population with a low rate of recent star formation. Surrounding the bulge, a faint, greenish disk component is visible. The disk exhibits a slightly mottled texture. Overall, the galaxy shows no major signs of tidal disturbances or ongoing major mergers, although there are subtle irregularities suggestive of minor interactions. The system likely possesses a significant stellar mass and a relatively low specific star formation rate.
