The galaxy exhibits an overall elongated, somewhat fusiform morphology suggestive of a spiral galaxy viewed at a high inclination, or perhaps a lenticular galaxy. The central region displays a bright, concentrated bulge, indicative of a significant stellar population and potential supermassive black hole activity. The bulge exhibits a yellowish-orange hue, consistent with an older stellar population dominated by evolved stars.

Extending outward from the bulge are fainter, bluish-white regions, possibly indicating the presence of a galactic disk. These bluer regions are suggestive of younger, hotter stars and ongoing star formation. The distribution of the blue light appears somewhat patchy and irregular, which could indicate spiral arm structures or star-forming regions within the disk. The galaxy appears relatively smooth in overall texture, with limited evidence of significant dust lanes or prominent star-forming knots that would typically be observed in actively star-forming spiral galaxies. The galaxy does not exhibit obvious signs of major mergers or tidal disturbances, though subtle irregularities in the disk might suggest minor past interactions.