The galaxy presents as a faint, elongated structure with a high degree of inclination, appearing nearly edge-on from our line of sight. A prominent central bulge is discernible. The bulge exhibits a moderate degree of roundness. The disk component appears smooth, with no readily apparent spiral arm structure visible. The overall color profile of the galaxy leans toward redder hues, particularly within the central bulge, suggesting an older stellar population or dust obscuration. There is no indication of any major mergers or tidal disturbances in the galaxy's morphology.
