The galaxy presents a largely smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a bright, compact core. Fainter, more diffuse light extends outwards from the core, forming a halo-like structure with a somewhat round shape. There is a subtle color gradient visible, with the core showing a warmer, yellower hue, and the outer regions appearing slightly bluer. The overall structure suggests a relatively evolved stellar population, consistent with a quiescent galaxy exhibiting low levels of star formation. There is no strong indication of spiral arms or prominent dust lanes. Subtle visual disturbances could indicate a minor past or ongoing interaction.
