The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of concentration, appearing as a bright, unresolved core. Moving outward from the core, the light intensity diminishes gradually, suggesting a smooth transition from the bulge to the outer regions of the galaxy. There is a slight elongation visible, indicating a deviation from a perfectly circular shape. Overall, the galaxy shows no obvious signs of distinct spiral arms or strong tidal disturbances, indicating it may be a relatively undisturbed system. The color profile appears relatively uniform, trending towards a redder hue, which suggests a stellar population dominated by older stars. No strong evidence of active star formation regions is readily apparent.
