The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, exhibiting a moderate axis ratio. The central region of the galaxy displays a higher surface brightness, suggesting a concentrated stellar population or active galactic nucleus. The color profile indicates a redder hue in the core region, transitioning to slightly bluer shades in the outer regions. There is a faint hint of disk like morphology. There appears to be some minor disturbance or possible merger in its morphology.
