The galaxy presents as a centrally concentrated, luminous object. It appears to have a generally smooth morphology. A central, bright core dominates the light profile, surrounded by a fainter, more diffuse halo. The halo exhibits a subtle blue tint, suggesting the presence of younger stellar populations and ongoing star formation, albeit at a moderate rate. There seems to be minor structural irregularity along the top portion of the galaxy. The galaxy is likely a massive system.
