The galaxy exhibits a distinct disk morphology, oriented nearly edge-on relative to our line of sight. A prominent central bulge is visible, appearing smooth and spheroidal. The color of the bulge suggests an older stellar population compared to the disk. The disk component shows some degree of structure, hinting at the presence of dust lanes obscuring regions of star formation. However, these features appear subtle. There are no significant signs of recent merger events, though the disk morphology suggests that some minor interactions may have occurred in the past. Overall, this galaxy appears to be relatively evolved.
