The galaxy presents as an elongated, edge-on spiral system. A prominent, relatively large bulge dominates the central region, exhibiting a yellowish-orange hue, indicative of an older stellar population. This suggests a history of significant star formation that has since slowed.

Extending from the central bulge are fainter, blue-tinged disk components. These appear relatively smooth, hinting at a well-established disk structure, although there may be some subtle disturbances present within the disk region. The blue color suggests the presence of younger, hotter stars indicative of active star formation, albeit at a moderate rate.

The absence of any clearly defined spiral arm structure or significant dust lanes suggests a relatively evolved system, possibly with a lower gas content. There is no obvious evidence of any major merging activity or tidal distortions. The bulge appears rounded and does not exhibit boxy features.
