The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a high degree of concentration, indicating a dense stellar population, likely composed of older, redder stars. The isophotes appear mostly regular, suggesting a relaxed dynamical state, although a slight deviation from perfect ellipticity is observable. The galaxy appears to be transitioning from a smooth, spherical shape towards a more in-between, slightly elongated form. There's no clear indication of a prominent disk component or spiral arm structure, and no significant dust lanes or major morphological disturbances are apparent, pointing to a possible quiescence in recent merging activity. The galaxy's overall color is yellowish, which is consistent with a dominant population of evolved stars. The size appears typical for an elliptical galaxy at a moderate redshift. Star formation rate is most likely low within the galaxy.