The galaxy appears to be an elliptical type, presenting a smooth, largely featureless morphology. Its overall shape is generally round, with minimal deviation from circularity. The light distribution is concentrated towards the center, with a gradual decrease in intensity extending outwards. There is no evident spiral arm structure or defined dust lanes visible. A faint halo of diffuse light surrounds the core region. There is a slight indication of a minor disturbance or interaction, but it is difficult to ascertain from the image alone whether this is a true merging event or a minor tidal effect. The galaxy exhibits a central region of bright luminosity.
