The observed galaxy presents as an edge-on spiral. The disk appears elongated, with a noticeable bulge that is rounded in morphology. The galaxy exhibits a central concentration of light, decreasing outwards toward the edges of the disk. The galaxy is oriented nearly perpendicular to the line of sight. There is no evidence of recent major merging activity or significant tidal disturbances, though the galaxy cannot be completely ruled out as a merging galaxy. There is no clear evidence of resolved spiral arms or dust lanes within the disk structure in this image. The galaxy appears relatively smooth in texture along the disk.
