The observed galaxy presents as an edge-on or highly inclined disk galaxy. A prominent dust lane bisects the galaxy's major axis, obscuring light from the central bulge region. The bulge appears centrally concentrated and rounded, and its color suggests an older stellar population, though some star formation appears to be occurring within the disk. Evident disturbances appear in the galactic morphology, particularly around the dust lane, indicating possible minor interaction with another galaxy or other galactic merger or accretion. The overall color profile indicates significant ongoing star formation, classifying this as a star-forming galaxy.
