The galaxy presents as a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge that graduates into a fainter halo. The light distribution suggests a relatively evolved stellar population, with a concentration of older, redder stars dominating the galactic center, evidenced by the yellowish-orange hue. There may be a sign of very minor disturbance, possibly due to a small tidal interaction, or it may be an artifact. Overall, the galaxy's color and morphology point to a galaxy with a relatively low ongoing star formation rate.
