The galaxy appears as a relatively smooth, elliptical structure, exhibiting a central concentration of light. Its overall shape approximates a rounded form, with only minor deviations from perfect circularity. The light profile transitions smoothly from a bright, yellowish core outwards, suggesting an older stellar population dominating its composition. There are faint, diffuse extensions beyond the central region, indicating a more extended galactic halo. There is little evidence of spiral arms or significant dust lanes within the galaxy, and no major signs of ongoing mergers. Overall, the galaxy exhibits characteristics consistent with an evolved, relatively quiescent system.
