The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue. The overall shape is somewhere between round and elliptical. There is no significant evidence of prominent spiral arms or strong tidal features, though a subtle extension or faint asymmetry might be present in the outer regions of the galaxy. The color gradient suggests an older stellar population dominates, consistent with a low star formation rate. Any signs of recent mergers or major disturbances appear to be minimal.
