The galaxy presents a generally smooth, elliptical morphology. It appears nearly spherical, with a high degree of central concentration. The light profile suggests a lack of prominent spiral arms or a well-defined disk structure. The galaxy exhibits a color gradient, appearing more yellow-orange toward the core, possibly indicating an older stellar population in the central regions. There is no immediately obvious evidence of tidal features, major mergers, or significant dust lanes from what is visible. The light is relatively evenly distributed with a high degree of light concentration in the center, and the absence of blue regions hints at a low ongoing star formation rate.
