The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated with a gradual falloff in intensity towards the outer regions. Color gradients are subtle, with the central region exhibiting a yellowish hue, potentially indicative of an older stellar population. The overall shape is moderately elongated, suggesting a departure from perfect spherical symmetry. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although the possibility of minor interactions cannot be ruled out. Based on its morphology and color, it is likely a massive galaxy that has largely ceased active star formation.
