The galaxy presents as a smooth, round, and relatively undisturbed structure. It appears to be an elliptical galaxy due to the absence of spiral arms or a defined disk. The light distribution suggests a high degree of central concentration, diminishing gradually toward the outer edges.

The galaxy exhibits a yellow-red hue, indicative of an older stellar population with a low rate of star formation. The even color distribution across the galaxy reinforces the absence of young, blue stars usually associated with active star-forming regions. There is no apparent dust lane or prominent features to suggest recent or ongoing merger activity, although subtle asymmetry cannot be ruled out due to the limitations of the image resolution.
