The galaxy presents as an elliptical or lenticular morphology, displaying a smooth, concentrated light profile. A noticeable absence of distinct spiral arms or prominent dust lanes is apparent. The color gradient suggests a redder hue concentrated towards the core, possibly indicating an older stellar population in the central region. The overall symmetry appears largely undisturbed, with no obvious signs of recent major merger events or significant tidal distortions. There is a slight hint of a surrounding halo, though not clearly defined. Based on the red color, it shows a low rate of star formation.
