The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white color, suggesting a population of older stars. Surrounding the core is a more diffuse, greenish-blue region, which may indicate the presence of some ongoing star formation. The galaxy appears largely undisturbed with no clear evidence of a major merger event. A slight asymmetry is noted in the distribution of the outer blue region, though this could result from tidal interactions or intrinsic structural features within the galaxy. The overall round appearance suggests it is likely an elliptical or S0 galaxy.
