The galaxy presents as a relatively smooth, disk-like structure. The central bulge exhibits a concentrated brightness, appearing largely spheroidal and intensely luminous. Extending outward from the bulge, a flattened disk is visible, exhibiting an almost edge-on profile. There are some disturbances and asymmetries in the morphology, but overall, the structure appears well-formed. Some low-level tidal features are visible in the surrounding space, suggesting potential past minor interactions. The overall color suggests a well-established stellar population, leaning toward a redder, more evolved population in the core, possibly a reduction in active star formation. Some minor disturbances on the edge of the disk suggest that this is not a perfectly relaxed system.
