The galaxy presents a roughly circular morphology. The central region exhibits high surface brightness, appearing as a concentrated, bright area. The color of the central region appears to be a relatively homogenous blue-white, potentially indicative of a population of young, hot stars. Fainter, slightly elongated structure is visible extending outward from the central region. The outer regions of the galaxy show a gradual decline in surface brightness, with a bluish hue. There is some indication of subtle irregularities in the outer structure that suggests some sort of disturbance, perhaps tidal effects from a minor merger. The overall form suggests that the galaxy is undergoing some kind of active evolution.
