This galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a high degree of luminosity, suggestive of a dense concentration of stars or potentially an active galactic nucleus. Moving outward from the core, the intensity of light decreases gradually, forming an extended halo with a hint of a disk shape. The color profile appears to be skewed towards the redder end of the spectrum indicating an older stellar population. There are no distinctly visible spiral arm structures or significant dust lanes within the galaxy's morphology, suggesting a more evolved state. There appears to be no significant disturbance in the galaxy indicating there are no signs of recent or ongoing major merger activity. Faint blue light at the edges indicate there are some areas of recent star formation within the galaxy.
