The galaxy appears as a concentrated, yellowish-white spheroid. Its morphology is largely smooth with minimal discernible features. There is some evidence of slight extension from the center, and some deviation from perfect circularity. The core is comparatively bright, suggesting a high concentration of stars and/or an active galactic nucleus. There are no immediately apparent indications of spiral arms or a prominent disk structure; instead, the galaxy presents as an elliptical-like system with a relatively uniform luminosity gradient from the center outwards. The overall appearance suggests a more evolved stellar population and a relatively low ongoing star formation rate. There does not seem to be significant recent merger activity, although the galaxy could be exhibiting minor disturbances.
