This galaxy exhibits a somewhat elongated morphology. The primary body of the galaxy displays a smooth light distribution. The central region appears brighter and slightly yellowish, potentially indicating a higher concentration of older stellar populations or dust obscuration. Extending from one side of the main body, there is a fainter, less defined feature. This could be a tidal tail, a disrupted arm, or an area of active star formation, the bluer color being suggestive of the latter. The overall structure suggests a galaxy that may have experienced or is currently undergoing some form of interaction or disturbance, but the system does not look strongly disturbed. The smoothness suggests a well-mixed older population, but the offshoot seems to contrast that idea. Further investigation of this galaxy would be of high interest.
