The galaxy appears as a central, diffuse light source with a generally elliptical morphology. The color gradient suggests a relatively uniform stellar population, possibly indicative of an older galaxy with limited ongoing star formation. The galaxy's apparent size is relatively small in the image, hinting at a considerable distance. There are no prominent spiral arms or dust lanes visible, leading to the preliminary classification of a possibly lenticular or elliptical galaxy. Faint disturbances may be present, possibly indicating a minor merger event. The object is generally smooth in appearance, with no obvious signs of active galactic nuclei activity or bright, knotty star-forming regions. The overall color appears to be skewed toward the redder end of the spectrum.
