The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears to gradually decrease from the center outward, lacking prominent spiral arms or distinct features usually associated with late-type galaxies.  The shape is mostly round, with a slight deviation towards an elongated form. There's no visually apparent ongoing major merger activity or significant tidal disturbance, although subtle irregularities in the outer regions might suggest minor interactions or past disturbances. Based on the color index, there is a redder hue indicative of an older stellar population with lower levels of current star formation. 
