The galaxy presents a moderately disturbed morphology, possibly indicating an ongoing or recent interaction. The central region exhibits a bright, relatively smooth structure, suggestive of an evolved stellar population. A fainter region, with a more diffuse and potentially active star-forming component, is visible nearby. The overall shape appears to be somewhat elongated, possibly indicating tidal distortion. The galaxy's moderate redshift suggests a significant distance, contributing to the blurring of finer details.
