The galaxy appears as a moderately bright, elliptical object. Its light is concentrated towards the center, exhibiting a smooth profile with no prominent spiral arms or distinct features immediately apparent. There may be a subtle disklike structure. The galaxy exhibits a mostly yellow hue, which suggests an older stellar population with minimal ongoing star formation. Based on the color index, the galaxy appears to be more luminous in redder wavelengths than in bluer wavelengths. There is no evidence of major mergers or significant tidal disturbances. The image suggests that this is a relatively massive galaxy.