This galaxy presents a generally smooth, elliptical appearance. There may be a slight disk-like structure, but it is faint, obscured by the dominant central bulge. The color profile indicates a population of older stars with a reddish hue. There is a slight asymmetry, possibly indicating a minor gravitational disturbance. The galaxy displays a notable central concentration of light and color, suggesting a denser population of stars or an active galactic nucleus. The galaxy does not exhibit strong evidence of ongoing, significant star formation.
