The galaxy presents a generally smooth morphology, with a luminous central bulge that is distinctly bright yellow. The light appears to fade outward from the core, transitioning into fainter orange hues at the galaxy's periphery. There's a possible slight flattening of the disk, and subtle asymmetry, but there is no evidence of strong spiral arm structure or significant dust lane features within the limitations of the image resolution. There are hints of possible disturbances. The color suggests an older stellar population and potentially low levels of ongoing star formation. The galaxy's shape appears to be somewhere between round and elliptical.
