The galaxy appears as a centrally concentrated system with a relatively smooth morphology. The light distribution suggests a lack of prominent spiral arms or a well-defined disk structure. The core exhibits a yellowish hue, gradually transitioning to bluer tones in the outer regions. There are some faint structures within the bluer regions, that may be due to some star formation or slight perturbations. Overall, the galaxy exhibits a shape that is neither perfectly spherical nor elongated, and does not show signs of significant tidal disturbances or interactions.
