The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentration of light, appearing more luminous than the outer regions. The color profile suggests an older stellar population, tending towards redder hues, although there appears to be traces of star formation. The overall morphology appears largely undisturbed. The galaxy displays an intermediate roundness. There may be a minor disturbance as the galaxy could possibly be merging with another object nearby. 
