The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There is a noticeable color gradient, transitioning from a brighter, yellowish core to a redder, less luminous outer region. The light distribution appears largely uniform without distinct spiral arm features or prominent dust lanes, suggesting an older stellar population. The galaxy exhibits a high degree of rotational symmetry. The overall shape can be described as moderately elongated. There are no obvious signs of recent or ongoing major mergers or tidal disturbances.
