The galaxy exhibits a flattened, disk-like morphology, but the orientation is neither face-on nor edge-on, rather at an intermediate angle. The central region presents a bright, concentrated bulge or nucleus. Proceeding outward, the galaxy shows a more diffuse distribution of light. Faint arm-like structures may be present, however they are indistinct. There appears to be limited ongoing star formation in the galaxy, particularly near the center. The overall color index suggests a relatively evolved stellar population. There appears to be some minor tidal disturbance in the galaxy, evidenced by the asymmetric distribution of light in the outer regions. The galaxy does not appear to be undergoing a major merger.
