The galaxy appears as a distorted spiral, potentially an elliptical galaxy. It exhibits a relatively smooth central region with a noticeable elongation, giving it a somewhat cigar-like shape. Faint tidal streams are visible extending from the main body of the galaxy, hinting at possible past interactions or merger events. These streams suggest some ongoing gravitational disturbance within the system. The color profile indicates a generally older stellar population, with a redder hue dominating the galaxy's overall appearance. The central regions seem somewhat brighter and more concentrated. 
