The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-spherical morphology, with a slight deviation towards an elliptical shape. A bright central bulge dominates the galaxy's luminosity profile, surrounded by a fainter, more diffuse halo or disk component. The color gradient suggests a blueish hue, which may indicate the presence of younger stellar populations and ongoing star formation, though this appears to be happening at a low rate. There is no apparent evidence of major tidal disturbances or active galactic nuclei activity.
