This galaxy exhibits a lenticular morphology, appearing as a flattened disk viewed at a significant inclination. The central bulge is prominent and exhibits a smooth, concentrated distribution of light, suggesting an older stellar population. The disk component shows a bluer hue compared to the bulge, indicating ongoing or recent star formation within its spiral arms. Faint dust lanes are suspected within the disk, although high inclination hinders clear observation. No apparent major merger events are observed, though subtle asymmetries in the disk could indicate minor tidal interactions. The galaxy shows signatures of active star formation. HI properties are measured, indicating a significant amount of neutral hydrogen present.
