The galaxy presents as a centrally concentrated object with a generally smooth morphology. There appears to be a radial gradient in luminosity, decreasing from the core outwards. The color profile is relatively uniform, with a slight shift towards redder hues in the outer regions of the galaxy. The overall shape is close to elliptical, displaying a moderate degree of roundness, with no apparent signs of strong tidal disturbances or ongoing major merger activity. Subtle asymmetries or minor disturbances cannot be entirely ruled out. The galaxy does not display any prominent spiral arm structures or a clear disk component at this resolution.
