The galaxy presents as a luminous, elliptical structure with a high degree of central concentration. It appears largely featureless, displaying a smooth, diffuse light distribution without prominent spiral arms or distinct dust lanes. The overall color is slightly red-shifted, leaning towards a warmer, yellower hue. The roundness is quite pronounced. There is no obvious indication of ongoing major mergers or significant tidal disturbances. The estimated size is relatively small, however, the luminosity is quite high. Despite the absence of prominent features, there might be evidence of minor disturbances upon further analysis. The star formation rate appears to be low, suggesting a population dominated by older stars.
