The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light profile appears to gradually decrease in intensity from the core outwards, with no prominent spiral arms or distinct features immediately apparent. The overall shape is elongated, but not excessively so, tending towards a more intermediate ellipticity. There may be a slight disturbance or minor irregularity in the outer regions of the galaxy, but the galaxy is not undergoing a major merger, and shows no other substantial evidence of strong gravitational interactions. The color distribution appears relatively uniform with a slight shift towards redder hues at the center and bluer hues towards the outer edges. I would assume this galaxy is not very actively forming stars. 
