This galaxy appears to be a lenticular or possibly a spiral galaxy viewed edge-on. It exhibits a flattened, elongated morphology, resembling a cigar shape. The galaxy's light is concentrated towards the center, suggesting a central bulge. There is some evidence of a disk component, however it is relatively smooth and featureless. The galaxy displays a noticeable color gradient, with the central regions appearing redder than the outer parts, which may indicate a higher abundance of older stars in the bulge compared to the disk. There are indications of weak ongoing star formation within the disk. The overall structure appears relatively undisturbed with no obvious signs of any major merger events. 
