The galaxy presents an elliptical morphology, appearing as a smooth, concentrated distribution of light. There are minimal signs of spiral arm structures or prominent dust lanes; it lacks significant distinct internal features. Its shape can be classified as moderately elliptical, tending toward round, with a slight deviation from a perfect sphere. There are no obvious indications of major mergers or significant tidal disturbances; the galaxy exhibits a generally undisturbed structure. The color profile suggests the presence of older stellar populations, indicated by a reddish-yellow hue. Overall, the galaxy appears to be a relatively quiescent system undergoing minimal star formation.
