The galaxy presents an overall elliptical morphology, appearing smooth and relatively featureless. There may be a slight elongation, suggesting a deviation from perfect circularity but it is still generally round. The central region exhibits a brighter, more concentrated luminosity, potentially indicative of a galactic nucleus. A gradual decrease in brightness is observable from the center towards the outer edges. The galaxy displays a color gradient, with a yellowish or reddish hue dominating the central region, transitioning to a bluer tint towards the periphery. This color variation suggests differences in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars more prevalent in the outer regions. There is no evident disk structure, spiral arms, or bar, and it appears there is no interaction with another galaxy.
