The galaxy presents a generally smooth and rounded morphology. The light distribution appears mostly homogenous, lacking prominent spiral arm structures or a distinct central bulge. The color indices suggest a population of older stars and a lack of significant ongoing star formation, correlating with the smooth appearance. There is a slight hint of asymmetry or possible minor tidal disturbance along its edges, indicating potential past or ongoing gravitational interaction, though it does not present as a merger. The core of the galaxy appears to be slightly brighter. Its form is generally elliptical. 
