The galaxy appears to be a relatively smooth, disk-shaped galaxy seen edge-on. It displays a moderate degree of elongation. The central bulge is prominent, exhibiting a concentrated bright intensity in shorter wavelengths, suggesting a significant population of older stars. There is a slight indication of a dust lane visible along the major axis, causing some obscuration of light from the central region. Overall, the galaxy's profile is quite regular, and there is no strong evidence of recent major merger activity or significant tidal disturbance.
