The galaxy appears as a centrally concentrated, generally smooth object. It displays a moderately elliptical morphology, close to circular in shape. The core exhibits high luminosity, suggesting a dense population of stars.

A subtle color gradient is observed, with a slightly bluer hue in the outer regions compared to the more yellow-white central bulge. This suggests a younger stellar population is present in the outer regions. Faint hints of what might be spiral arm structures may be present but not clearly defined. There is a lack of significant dust lanes or distinct features, indicating a relatively quiescent state. No obvious signs of active galactic nuclei activity or ongoing major merger events are readily apparent from the morphology. The overall appearance is consistent with an early-type spiral galaxy or a lenticular galaxy viewed at a moderate redshift.
