The galaxy appears as an elliptical-like structure, with a smooth, diffuse light profile. The central region exhibits a more concentrated and slightly brighter luminosity than the outer regions.

It presents a noticeable elongation, exhibiting a major-to-minor axis ratio of approximately 2:1. The color gradient indicates a centrally concentrated population of older stars, and a more extended distribution of younger stars in the disk. There is a slight disturbance in the outer disk, with irregular clumps of stars, but overall the structure is relatively smooth.
