The galaxy presents as a relatively compact, elliptical morphology, exhibiting a dominant bulge component with a smooth light distribution. There is a subtle transition from a more concentrated core to a gradually fading halo. The color gradient suggests a redder population of stars dominating the central regions, potentially indicating older stellar populations or dust obscuration. Some bluer regions are present towards the outer areas, perhaps indicating ongoing star formation, but these areas are sparse. There are no clear spiral arm structures or other prominent features like bars. Overall, the galaxy appears largely undisturbed, without obvious signs of major mergers or tidal interactions.
