The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The light distribution appears radially symmetric, indicating a lack of prominent spiral arms or a well-defined disk structure. The core exhibits a bright, diffuse glow that fades gradually towards the outer regions of the galaxy. There is a slight color gradient from a more yellow-red core, suggestive of an older stellar population, transitioning to bluer hues in the outer halo. The overall appearance indicates a gravitationally relaxed system with minimal signs of recent mergers or tidal disturbances. There are no distinct features of star formation visible. The structure does not suggest strong evidence of recent or ongoing interactions.
