The galaxy presents an elongated, spindle-like morphology, suggestive of an elliptical or lenticular type, seen nearly edge-on. A pronounced central bulge exhibits a bright, yellowish hue, indicative of an older stellar population. The outer regions, though less distinct, display a subtle disk-like structure. There appears to be a dust lane obscuring part of the central bulge along its major axis. Faint and indistinct features hint at some star formation. Overall the galaxy appears relatively undisturbed, showing no strong signs of recent merger activity.
