The galaxy presents as a centrally concentrated object, appearing largely smooth and elliptical in shape. There is no prominent disk structure or spiral arm morphology visible. The core exhibits a bright, yellowish hue, suggesting a significant population of older stars. The galaxy appears more luminous in redder wavelengths. The outer regions of the galaxy gradually fade into the background, showing no distinct features or sharp boundaries. There's a very slight asymmetry in the outer halo, but overall it appears relatively undisturbed with no signs of major mergers or tidal interactions. The color gradient suggests possible ongoing, but low, star formation activity.
