The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears relatively uniform, lacking prominent spiral arms or a well-defined bar structure. The galaxy exhibits a slightly elliptical shape. The overall color of the galaxy appears to be on the redder end of the spectrum, suggesting an older stellar population and/or a significant dust component. There are no obvious signs of recent major merger activity, though some minor disturbances cannot be ruled out at this resolution. The light distribution suggests a classification leaning towards an early-type galaxy, possibly an elliptical or lenticular galaxy.
