The galaxy appears as a centrally concentrated, relatively smooth object. Its morphology is largely spheroidal, exhibiting little evidence of spiral arms or a prominent disk structure. The light distribution suggests a well-defined core with a gradual decrease in luminosity outward. There is a slight elongation, but the galaxy is generally round in appearance. The color profile indicates a subtle reddening towards the center, potentially indicative of an older stellar population or increased dust concentration. Faint, diffuse light extends slightly beyond the main body of the galaxy. There is no visual indication of ongoing major mergers or significant tidal disturbances in this image.
