The galaxy presents as a somewhat elliptical, disk-like structure. A central bulge is evident with a yellowish hue, suggesting an older stellar population. The main body of the galaxy is elongated, displaying an axis ratio indicating a deviation from perfect circularity. There is a slight asymmetry in the galaxy's overall shape. It doesn't appear to be a pure elliptical, there seem to be some disrupted features. A fainter, diffuse region appears adjacent to the main galactic body, potentially indicating either tidal interactions or satellite galaxies. There is no strong evidence of spiral arm structure, although the bluer edges suggest active star formation in a disk, though it appears quite disordered.
