The galaxy presents as an edge-on disk galaxy with a prominent bulge. The disk exhibits a degree of dust lane obscuration, bisecting the galaxy's light. The bulge appears smooth and rounded, dominating the central region. The disk shows a relatively uniform color gradient from the bulge towards the edge, indicative of an aging stellar population. There is a hint of bluer regions within the galaxy. These may indicate pockets of star formation or younger stellar populations. The overall morphology suggests a quiescent system with minimal interaction. The galaxy is relatively compact with an elliptical appearance. 