This galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. The galaxy exhibits a color gradient, with a yellowish-white core that transitions to redder hues in the outer regions. There is no distinct spiral arm structure visible. Minor disturbances may be present, but do not seem to largely affect the smooth structure. The intermediate roundness of the galaxy suggests that it is likely an elliptical, possibly an E4 or E5 on the Hubble scale. Star formation activity appears to be low, as inferred from the redder overall color of the galaxy. This observation indicates a population dominated by older, redder stars. No signs of a major merger or significant tidal interactions are apparent.
