The galaxy presents as a smooth, centrally concentrated object with a nearly circular morphology. There is no visible disk structure or spiral arm features evident in this image. The light distribution appears relatively uniform, lacking distinct clumps of star formation regions. The color gradient suggests a dominant older stellar population, with a redder hue, and minimal presence of dust lanes obscuring the central region. There are no apparent signs of recent merger activity or tidal disturbances based on the smooth light profile.
