The galaxy presents as a relatively compact object. Its morphology appears generally smooth with a high degree of roundness. The galaxy exhibits a bright, concentrated core which indicates a significant stellar population. The color profile appears somewhat uniform across the galaxy, with a subtle yellow-orange hue suggesting an older stellar population and less active star formation. There is no strong indication of spiral arms or a prominent disk. The overall appearance suggests it may be an elliptical galaxy. There is no visual evidence of ongoing major mergers or tidal disturbances, though subtle, minor disturbances cannot be ruled out. The galaxy's estimated size indicates that it is a galaxy of considerable extent.
