The galaxy presents a relatively smooth morphology, although some irregular features are discernible. Its overall form is somewhat rounded, but not perfectly spherical, displaying a slight elongation. A central concentration of light suggests a possible core or bulge region. The galaxy exhibits a color gradient, with the central region appearing more yellow/orange, potentially indicating an older stellar population, while the outer regions show a hint of bluer hues, which could signify the presence of younger, hotter stars or ongoing star formation. There are faint wispy extensions emanating from the main body of the galaxy, potentially indicating tidal features or disrupted structures, suggesting a possible interaction or merger event.