The galaxy presents a generally smooth and rounded appearance. There may be a slight hint of disk-like structure, but it is faint. The light is more concentrated toward the center of the galaxy and diffuses towards the edges, with an elliptical shape to the distribution. A yellowish hue dominates the light emitted, implying an older stellar population and lower ongoing star formation rate. There is no clear evidence of strong tidal disturbances or ongoing major mergers.
