The galaxy appears as a moderately bright, elliptical-shaped object with a smooth, featureless morphology. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. The color profile suggests a relatively evolved stellar population, indicated by the yellow-orange hue. There is no readily apparent spiral arm structure or significant dust lane obscuration. There may be minor distortions, suggesting a possible gravitational interaction, but no major mergers are observed. The object has a moderate size.
