The galaxy appears as an elliptical or spheroidal system, exhibiting a smooth, relatively featureless morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions, lacking prominent spiral arms or a distinct disk structure. The color profile suggests a population of older stars, indicated by the reddish-yellow hue, and a lower rate of recent star formation activity. There is no obvious evidence of ongoing mergers or major tidal disturbances based on the galaxy's overall structure. The shape is generally rounded. The galaxy is moderately bright, suggesting substantial mass and luminosity.
