The galaxy appears to be a relatively compact and luminous object. Its overall morphology is smooth and elliptical, with a high degree of central concentration. The color profile suggests a population of older stars, appearing redder in the composite image. There is a faint hint of a possible tidal interaction or minor disturbance in the form of a small feature or faint plume emanating from the main body of the galaxy, perhaps indicative of a past or ongoing minor merger event. The galaxy's apparent roundness suggests it is viewed close to face-on. There does not appear to be significant dust obscuration or active star formation within the galaxy itself.
