The galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a high degree of central concentration, with a bright, almost stellar-like nucleus dominating the visual appearance. The light profile fades gradually from the core, suggesting a lack of significant spiral arm structure or prominent dust lanes. There is no apparent ongoing major merging activity, but there may be some minor irregularities or disturbances in the outer regions, possibly indicating past interactions. The color of the galaxy appears relatively uniform, with a slight shift towards redder wavelengths, typical of older stellar populations. Based on its apparent smoothness and color, the galaxy may be an early-type system dominated by evolved stars with little ongoing star formation. It is generally round in shape.
