The galaxy appears to be a spiral galaxy viewed at a significant angle. It exhibits a central bulge region that is quite prominent and bright, suggesting a high concentration of stars, likely older populations. The bulge is roughly elliptical in shape. Emanating from the central bulge is a fainter, somewhat indistinct disk. There is some evidence of spiral arm structure within the disk, although it lacks sharp definition. Overall, the galaxy has a smooth, almost featureless appearance, with a slightly elongated shape. The color of the galaxy appears to be generally yellow-white, indicating a mix of stellar populations, potentially with a slightly higher proportion of older, redder stars compared to younger, bluer stars that are found in galaxies with active star formation.
