The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The central region exhibits a brighter, more intensely luminous core, possibly indicative of a supermassive black hole or a high density of stars. Moving outwards from the core, the light gradually diffuses, suggesting a decreasing stellar density. There is a subtle color gradient, with the core appearing slightly redder or yellower, and the outer regions exhibiting a bluer hue. This color variation may reflect differences in stellar populations, with older, redder stars dominating the core, and younger, bluer stars being more prevalent in the outer regions. The overall structure appears undisturbed, lacking any prominent spiral arms, bars, or signs of recent mergers. The galaxy appears relatively isolated.