The galaxy presents as an elliptical morphology. Its light distribution is centrally concentrated and appears relatively smooth, lacking prominent spiral arms or distinct substructures. The shape is elongated, with an approximate cigar-like appearance, although not heavily so. The color gradient suggests an older stellar population, with a yellowish-orange hue at the core that transitions to a bluer outer region. There is no clear evidence of ongoing major merger activity, however there could be some minor disturbance in the outer regions. Overall, the galaxy appears as a fairly undisturbed, evolved system.
