The galaxy presents as a relatively smooth, centrally concentrated light distribution. It exhibits a generally elliptical morphology, approaching a circular shape, with minimal discernible features such as spiral arms or a prominent disk. The central region displays a bright, concentrated core, potentially indicative of a galactic nucleus. The light profile gradually decreases in intensity from the core outwards, suggesting a spheroid-dominated system. Faint, diffuse extensions are possibly present but not distinctly pronounced, lacking sharp edges. There are hints of a slightly bluer hue in the outer regions, while the core appears redder, which may be indicative of differing stellar populations or dust content between the center and the edges. There is no evidence of ongoing major mergers, significant tidal disturbances, or pronounced irregular structures.
