The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a lack of significant ongoing star formation, leaning towards an older stellar population. There's a smooth, gradual decline in luminosity from the core outwards, indicating a well-mixed stellar distribution. No apparent spiral arm structures or dust lanes are visible. The galaxy appears largely undisturbed, showing no signs of major merging events or tidal distortions. Overall, the morphology is consistent with that of a massive elliptical galaxy at an approximate distance corresponding to a redshift of around 0.3.
