The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a dominant, bright nucleus exhibiting a yellow-white hue, suggesting a population of older stars. The light diminishes gradually outwards from the core. The outer regions of the galaxy display a faint, diffuse glow, showing subtle extensions without any clear spiral arm structure or prominent dust lanes. Overall, the galaxy exhibits a high degree of symmetry and smoothness, characteristic of an early-type galaxy. There is a hint of faint blueish-white coloration in the galaxy, suggesting the presence of a small population of younger, hotter stars. The galaxy is not currently undergoing a major merger but the overall morphology displays some faint disturbances.
