The galaxy presents a largely smooth morphology. It is elliptical in shape, appearing nearly round. There is no strong evidence of a spiral structure or a prominent disk. A slight degree of irregularity is noticeable within the galaxy's outer regions, suggesting it could have experienced a minor disturbance. The color profile suggests a population dominated by older stars, with a redder overall hue. No active star forming regions or bright blue knots are apparent. The galaxy appears relatively isolated, without any nearby interacting companions.
