The galaxy presents as a centrally concentrated elliptical morphology. The core exhibits a bright, yellowish-white emission, suggesting a high concentration of older stellar populations and minimal dust obscuration in this region. Progressing outwards from the core, the color gradually shifts towards a redder hue, indicating an aging stellar population with potentially lower levels of recent star formation activity. The galaxy appears relatively smooth and symmetric, displaying no prominent spiral arms or distinct features indicative of ongoing major mergers or significant tidal disturbances. There is a very subtle extension in the galaxy's halo on the right, suggesting there could have been a minor merger in the past. 
