The galaxy presents as an edge-on spiral or lenticular system. A prominent bulge is visible, exhibiting a moderate degree of concentration. A disk is clearly apparent and is elongated, with evidence of dust lane obscuration along its mid-plane. The axial ratio of the disk suggests a substantial inclination angle relative to our line of sight. Some asymmetry is detected along the disk, possibly indicating minor tidal interactions or internal disturbances. The color gradient shows bluer colors towards the outer regions of the disk, potentially indicative of ongoing star formation. Overall, the galaxy exhibits a relatively smooth morphology, although with subtle features indicative of dynamical activity.
