The galaxy exhibits a generally elongated morphology. The primary body of the galaxy appears relatively smooth and centrally concentrated, showing a hint of elliptical structure. Extending from this central region is a fainter, somewhat diffuse feature. This secondary component suggests a possible tidal tail or a plume-like structure. The color of the primary body appears slightly redder in comparison to the tail-like structure, which has a bluer hue. This color variation might indicate differing stellar populations or dust content within these regions. Overall, the galaxy appears to be undergoing or to have recently experienced some form of gravitational interaction that could be responsible for the observed structure.
