The galaxy appears as a relatively compact object. The central region exhibits a bright, concentrated core, suggesting a high stellar density or active galactic nucleus. Surrounding the core is a less defined, somewhat diffuse halo. A slight asymmetry is visible in the outer regions, which may indicate a possible disturbance. A faint tidal tail is barely visible, potentially resulting from a minor merger or gravitational interaction with another galaxy. The dominant color is greenish, transitioning to bluish, particularly towards the outer edges. This color gradient may indicate differing stellar populations or dust content, with potential star formation occurring in these regions. Based on this appearance, the galaxy is most likely an elliptical galaxy with a small likelihood of being a merging spiral.
