The galaxy presents a flattened, disk-like morphology, viewed at an oblique angle, though not perfectly edge-on. It exhibits a central bulge that is brighter and more concentrated than the outer regions. The light from the central bulge appears yellowish, suggesting an older stellar population. Moving outwards from the bulge, the disk appears somewhat irregular with some clumpy structure. Traces of spiral arm structure may be present but are not well-defined. The outer disk regions show a bluer color, indicative of ongoing star formation. The overall shape appears moderately elongated, with the major axis extending approximately twice as far as the minor axis. There is no evidence of a strong bar structure. The galaxy appears relatively isolated, with no clear signs of major interactions or mergers.
