The galaxy presents as a generally smooth and centrally concentrated object. Its morphology is primarily spheroidal, with a gradual decrease in luminosity from the core outwards. There is no obvious spiral arm structure or bar feature visible within the limits of the observation. The color profile indicates a slightly redder core, transitioning to a more bluish hue in the outer regions, suggesting a presence of evolved stellar populations at the galactic center and a small amount of star formation in the outer regions. No major merger events are apparent, with no distinct tidal tails or asymmetric structural disturbances visible, though there may be some minor disturbances. The object appears relatively isolated and undisturbed. It has a moderate size in the image. 
