The galaxy presents as an edge-on spiral, characterized by a prominent, centrally located bulge. The bulge exhibits a smooth, rounded morphology with a yellowish hue suggesting an older stellar population. A faint disk extends outwards from the central bulge, displaying a slight inclination relative to our line of sight. The disk component presents some faint dusty features and a few possible areas of star formation. Overall, this galaxy appears to be relatively isolated, showing no signs of major disturbances.
