The galaxy presents as a relatively smooth, disk-like structure, viewed at a significant inclination. Its shape is elongated, with an apparent cigar-like morphology. The central region exhibits a higher concentration of light, appearing as a prominent bulge. The color gradient suggests a slightly older stellar population in the central bulge, with bluer hues in the outer disk. There is no obvious indication of strong spiral arm structure or major tidal disturbances, suggesting a relatively undisturbed and evolved system. There is a hint of faint dust lanes within the disk, though the limited resolution makes detailed analysis difficult. The galaxy does not appear to be actively merging, although very subtle disturbances are possible but difficult to confirm in this image.
