The galaxy presents as a relatively smooth and centrally concentrated system, exhibiting a somewhat elliptical morphology. The light profile appears to gradually decrease in intensity from the bright nucleus outward. There is a slight bluing in the galaxy disk compared to the yellow-shifted bright nucleus. No prominent spiral arm structures or distinct dust lanes are discernible in this image. The galaxy does not show obvious signs of significant tidal disturbances or ongoing major merging activity. The galaxy is more elongated in the horizontal axis than the vertical axis. 
