The galaxy presents a primarily smooth morphology, with a dominant central bulge. The overall shape appears mostly round, with only slight deviations from perfect circularity. There is little evidence of significant spiral arm structures or other disk-like features. The color distribution is centrally concentrated, with a yellowish hue that diminishes towards the outer regions. Patches of redder color are scattered around the galaxy, suggesting the presence of areas with possible ongoing star formation or older stellar populations enshrouded in dust. Overall, the galaxy seems to have had a history of little to no major mergers, with only minor disturbances visible.
