The galaxy presents as a centrally concentrated object, generally elliptical in shape, with a smooth overall appearance. The core region exhibits a bright, diffuse glow, likely due to a dense population of stars. Moving outwards from the core, the light gradually fades. 

There is some asymmetry in the light distribution which suggests that the galaxy might have experienced a minor interaction or disturbance in the past. It also looks like there might be a merger event occuring. The galaxy is a yellowish/reddish hue, which indicates that its stellar population is largely composed of older, redder stars, and suggests a lack of ongoing, significant star formation.
