The galaxy appears as a moderately bright, elliptical structure, with a smooth, diffuse light distribution. It exhibits a slight elongation, appearing neither perfectly spherical nor highly flattened. The core is relatively concentrated, but without an obvious distinct nucleus. There is evidence of redder light in the central region of the galaxy, which may indicate an older stellar population. Fainter, bluer regions are visible on opposite sides of the main body, possibly indicating recent star formation or active galactic nuclei activity. The smooth appearance suggests that any spiral arms or distinct features have either been disrupted, or were never present. There is no visual evidence of tidal tails or other significant disturbances, implying that there has been no recent major merger events. 
