The galaxy appears as a luminous, centrally concentrated object. Its overall morphology suggests an elliptical galaxy, exhibiting a smooth, spheroidal light distribution. The core is bright and concentrated. Moving outwards from the core, the light intensity gradually diminishes. No distinct spiral arms or prominent dust lanes are visible. There is a suggestion of asymmetry in the outer regions. The color profile seems relatively uniform across the galaxy. Some minor disturbance is also detected.
