The galaxy presents as a disk galaxy seen at an oblique angle, appearing somewhat edge-on. The central bulge is prominent and exhibits a smooth, relatively featureless appearance. The disk appears to be fairly well-defined and shows hints of spiral structure, although the arms are not sharply resolved. The galaxy displays a blue hue, suggesting the presence of younger, hotter stars and ongoing star formation. There is also evidence of some dust lanes within the disk. Overall, the galaxy appears to be in a relatively isolated state, showing no strong signs of major tidal disturbances or recent mergers with other galaxies.
