The galaxy presents as a relatively compact and luminous object. Its morphology appears predominantly smooth and elliptical, with a high degree of central concentration. The light distribution suggests minimal discernible spiral arm structure or significant dust lanes. The galaxy exhibits a gradual decline in surface brightness from the core outwards, with a roughly circular or slightly elongated shape. There are no obvious signs of strong tidal disturbances or ongoing major merger activity. Faint, diffuse features might indicate minor interactions or disturbances, but these are subtle. The color is a consistent blue green, suggesting a relatively homogenous stellar population. Overall, the galaxy seems to be a fairly regular elliptical galaxy with a smooth light profile and no prominent morphological peculiarities.
