The observed galaxy presents as a disk galaxy, viewed at a near edge-on angle. A prominent dust lane is visible, bisecting the galaxy's disk. The central bulge appears relatively bright and concentrated, with a suggestion of color variation indicating differing stellar populations or dust obscuration within the bulge itself. The galaxy displays a color gradient; the inner disk region exhibits bluer tones while the outer regions transition towards redder hues. Some minor tidal disturbances or interactions are weakly suggested, potentially indicative of a recent or ongoing minor merger event, although this requires further investigation. Overall, the galaxy's morphology suggests a spiral or lenticular type, with moderate levels of star formation activity, especially visible by the bluer regions.

