The galaxy presents as a somewhat disturbed system, possibly undergoing a merger or interaction. The primary component is a bright, relatively smooth and concentrated bulge region exhibiting a yellowish-white hue, indicative of an older stellar population. A secondary component is visible, showing a more irregular, elongated morphology. There appears to be a faint bluish bridge connecting these components, indicative of tidal forces and possible star formation due to compression of gas. Faint extensions of light are seen from the galaxy, potentially remnants of the interaction. Overall, the morphology is neither perfectly elliptical nor a well-defined spiral, suggesting ongoing dynamical processes.