The galaxy appears as a somewhat flattened, elliptical-like structure, possibly a lenticular galaxy seen at an oblique angle. The central region is significantly brighter and more concentrated, indicating a substantial galactic nucleus or bulge. The color is generally a slightly yellowish white, suggesting a population of older stars. There is a hint of a fainter, more diffuse disk surrounding the central bulge, however, no distinct spiral arm structures are obviously visible. There may be a slight warp or irregularity to the outer edges of the disk. Based on the lack of readily apparent star-forming regions, the star formation rate is likely low to moderate. No obvious signs of recent major merger events or significant tidal disturbances are observed in the image.
