The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The light distribution appears relatively even, lacking prominent spiral arms or strong dust lanes. The overall shape approximates a circular form. The central region exhibits a brighter, more compact core, suggesting a higher concentration of stars. There is subtle color variation across the galaxy. The central core seems to be slightly yellower, which might suggest an older stellar population in this region. Outward from the core, the galaxy displays a faint, bluish halo, possibly indicating the presence of younger, hotter stars or ongoing star formation. A subtle asymmetry can be seen at the outer edge of the galaxy. There are no obvious signs of tidal interactions, major disturbances, or a recent merger event.
