The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely featureless, lacking any distinct spiral arm structures or prominent dust lanes. The color profile suggests a population of older stars, with a central region displaying a bluer hue that may indicate some ongoing star formation. The galaxy exhibits a high degree of circular symmetry, and is not displaying any obvious signs of interaction or tidal disturbance. It appears to be in a relatively quiescent state, with a low rate of star formation. 
