The galaxy presents as a relatively concentrated object with a brighter, yellowish central region that appears spheroid-shaped. Diffuse blue light extends outward from the central region, suggesting the presence of ongoing star formation within the outer regions or spiral arms. The ellipticity of the galaxy suggests it may be an elliptical galaxy or a spiral galaxy viewed at an angle. The object exhibits a relatively smooth profile with a minor disturbance, or potential merger, occurring nearby. This distortion indicates that the system may have experienced gravitational interactions, influencing the overall morphology.