The galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population. The galaxy displays a yellowish hue, indicative of an older stellar population with fewer young, hot, blue stars. There's a hint of a faint, diffuse halo surrounding the central body, which gradually fades into the background. No distinct spiral arms or dust lanes are visible in this image. Based on its morphology, it could be classified as an elliptical galaxy, perhaps of type E3-E5 on the Hubble sequence, where it is more on the elliptical side than the spiral side, and is fairly round but not completely circular. The galaxy shows no obvious signs of interaction or recent mergers.
