The galaxy presents as an edge-on spiral, exhibiting a relatively bright central bulge that appears somewhat elongated. A distinct dust lane is visible, bisecting the galaxy horizontally and contributing to the overall redder color. The galactic disk appears relatively thin and faint, extending outwards from the bulge. There is the suggestion of a slight warping or disturbance in the disk's morphology, possibly indicating an interaction or recent merger event. Faint tidal features or stellar streams are not clearly visible, but the irregular appearance of the disk warrants further investigation into potential interactions. The color profile of the galaxy suggests a presence of both older stellar populations within the bulge and younger, bluer stars in the disk.
