The galaxy presents as a moderately bright, elliptical-like structure. It has a smooth, diffuse appearance with no discernible spiral arms or distinct features. The light is concentrated toward the center, suggesting the presence of a bulge. The galaxy exhibits a yellowish hue, possibly indicating an older stellar population with relatively low star formation activity. There is a slight elongation to the structure, but it is generally quite circular in form. No evidence of significant tidal disturbances or ongoing mergers is visible.
