The galaxy presents as an elongated, spindle-shaped structure, suggesting a likely classification as an edge-on spiral or lenticular galaxy. A notable dust lane is potentially observed along its major axis. The central bulge is poorly defined, exhibiting a smooth but not perfectly spherical morphology, possibly indicating a bar structure along the length of the galaxy. The stellar population appears diverse, with a central yellow-white distribution possibly indicating an older stellar population in the core. Hints of blue star formation activity are weakly present at the edges of the galaxy, potentially implying ongoing or recent star formation in the disk. No signs of tidal features or major mergers are apparent. The overall morphology is that of a relatively undisturbed system.
