The galaxy appears to be a relatively smooth, elliptical galaxy, elongated in shape, with a cigar-like appearance. The core of the galaxy exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars within that region. The outer regions of the galaxy display a gradual fading in luminosity, indicative of a decreasing stellar density as radial distance from the center increases. There is minimal evidence of distinct spiral arm structures or significant dust lanes within the galaxy. A slight color gradient is visible, with the core displaying a more yellow/red hue, potentially indicating a population of older stars, while the outer regions show a bluer tinge, possibly indicating a small amount of ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger event, however a possible minor disturbance might be occuring.
