The galaxy presents an overall elliptical morphology, appearing relatively smooth and lacking prominent spiral arms or a distinct disk structure. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The color gradient suggests a redder core, potentially indicative of an older stellar population and/or increased dust obscuration in the central region. The overall color profile suggests the galaxy is likely composed of older stars, but there is still some star formation. There appears to be some minor disturbances in the galaxy, and signs of a potential past merger event.
