The galaxy presents as a somewhat elongated, centrally concentrated object. The core exhibits a yellowish-orange hue, suggesting an older stellar population. Extending outward from the core, the galaxy appears to have a disrupted structure. There is a faint bluish feature that suggests a region of younger stars or ionized gas, indicative of recent or ongoing star formation. The bulk of the galaxy is smooth. Based on the degree of distortion and the presence of potential tidal features, it's possible this galaxy is undergoing an interaction or merger with another galaxy. Further spectroscopic analysis is required to confirm merger status and better characterize the stellar populations and kinematics within the galaxy.
