The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution indicates a high degree of central concentration, with a luminosity profile that gradually decreases outwards. The color profile suggests a population dominated by older stars, exhibiting a redder hue, particularly toward the galactic center. There are no obvious signs of recent or ongoing major merger events. Faint irregularities in the outer regions suggest possible minor disturbances or tidal interactions.
