The observed galaxy presents as an edge-on spiral, or possibly lenticular, galaxy. The disk is sharply inclined with respect to our line of sight. A prominent central bulge dominates the galaxy's light profile. The bulge appears relatively smooth and rounded. The disk component displays a relatively featureless morphology with only a slight indication of a dust lane or spiral arm structure near the mid-plane. The light from the bulge appears to be of an older stellar population, with yellow-red coloration. The disk component has a slightly bluer hue, possibly indicating a younger stellar population. The overall structure is smooth and regular, with no apparent signs of major tidal disturbances or ongoing mergers, though some minor distortions are possible.
