The galaxy appears as a luminous, centrally concentrated object with a relatively smooth morphology. The light distribution suggests a dominant bulge component, with a gradual decrease in intensity moving outward from the core. There is a slight elongation to the galaxy's shape, but it is generally more rounded than disk-like. There may be some minor disturbances or features that suggests a possible interaction with another object. The galaxy is relatively bright, likely indicative of a significant stellar population.
