The galaxy presents as a single, centrally concentrated object. The light distribution appears relatively smooth, with a noticeable lack of distinct spiral arms or a prominent galactic bar. The galaxy’s shape is roughly intermediate between circular and elliptical, with a slight elongation. There is no apparent strong tidal features or obvious signs of an ongoing major merger.

The galaxy's color profile indicates a redder overall hue. There is a hint of some internal structure suggesting possible minor disturbances or interactions. The concentration of light decreases smoothly from the center outwards.
