The galaxy appears as a centrally concentrated object, with an overall smooth morphology. There is a slight elongation noticeable. The color profile suggests it's largely composed of older stellar populations, with a redder hue dominating. There appears to be some blue light scattered throughout the galaxy, but it is concentrated towards the core and along the edges. This may represent regions of younger star formation activity. The galaxy's overall structure does not show any significant signs of a major merger, although there may be very slight disturbances present. The object's light appears to be concentrated within a radius of approximately 6 arcseconds.
