The galaxy exhibits a prominent bulge, visually smooth in texture. The galaxy is elliptical, with a high degree of central concentration. The color gradient suggests a stellar population primarily composed of older stars, with a yellowish to reddish hue dominating the central region. A subtle disk component may be present, indicated by the slight flattening of the galaxy's overall shape. There may be a possible weak presence of a small amount of star formation. There are no signs of active galactic nuclei. There is no indication of significant tidal disturbance or ongoing merger activity.
