The galaxy presents as a relatively smooth, elongated structure with a central concentration of light. There is a noticeable color gradient, shifting from a yellow-orange hue in the core to a bluer periphery. This color difference suggests a variation in stellar populations and/or dust content between the central region and the outer regions. The smoothness of the light distribution suggests the absence of prominent spiral arms or significant dust lanes. Morphologically, it likely falls somewhere between an elliptical and a lenticular galaxy, with a slight preference toward the elliptical type. There are some signs of minor disturbance or interaction.
