The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a yellowish hue, possibly indicating an older stellar population. Fainter, diffuse material extends outward from the core, forming a halo or envelope around the galaxy. There is a subtle color gradient, with the outer regions appearing slightly bluer compared to the core, which could suggest the presence of some younger stars in the galaxy's outskirts. There's no distinct spiral arm structure or prominent dust lanes visible, supporting the classification as an elliptical type galaxy. The galaxy is moderately luminous. There is no obvious sign of interaction or recent merger events. The overall structure appears relaxed and well-defined.
