The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing bright and diffuse. Moving outwards from the center, the light intensity gradually decreases, fading into a more indistinct outer halo. There is a subtle color gradient, with the core showing a slightly yellow-shifted hue, suggesting an older stellar population. Faint, diffuse blue regions are interspersed throughout the main body of the galaxy. There is no indication of significant spiral arm structure or ongoing major merger events. Minor disturbances or faint tidal features cannot be definitively ruled out at this resolution, but they do not dominate the overall morphology.
