The galaxy presents a largely smooth and centrally concentrated morphology, with a high degree of radial symmetry. The galaxy's light profile appears to be well-fit by a single component, suggesting a lack of prominent spiral arms or a well-defined disk structure. There is a central concentration of light that transitions smoothly into the surrounding halo.

The overall color profile is relatively uniform with a mostly white appearance transitioning into light blue. There are no noticeable dust lanes or distinct knots of star formation visible in the image at this resolution. There is no evidence of any major ongoing merger events or significant tidal disturbances. Faint, subtle irregularities in the outer regions cannot be ruled out, but the dominant impression is that of a relaxed system. The galaxy appears closer to a disk galaxy, but is relatively smooth. 
