The galaxy presents a largely smooth and centrally concentrated morphology. It appears as a luminous, round object with a gradual decrease in light intensity from the core outwards. There is no prominent disk structure or spiral arm features visible. The color profile suggests a dominant older stellar population, characterized by a yellowish hue, particularly concentrated in the central region. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. The faintness and lack of detail indicate a galaxy at a considerable distance. Based on the smooth morphology and color profile, it is likely an elliptical galaxy or potentially a lenticular galaxy viewed face-on.
