The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent dust lane is visible, obscuring a significant portion of the galactic plane and indicating the presence of interstellar medium. The bulge appears somewhat rounded and centrally concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component displays a bluish tinge, particularly towards the outer regions, potentially indicating ongoing star formation. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. The overall morphology suggests a relatively evolved and stable system.
