The galaxy in the image presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge dominates the structure, appearing smooth and concentrated with a yellowish-orange hue, suggesting an older stellar population. The disk itself is elongated and thin, also exhibiting a yellowish color consistent with older stars and dust. There is little visible evidence of spiral arm structure or active star formation. The bulge appears somewhat rounded, with no obvious boxy shape. The overall morphology suggests a relatively undisturbed galaxy, with no significant signs of recent or ongoing merger activity. The galaxy appears to be moderately massive, and its star formation rate is likely low.
