The galaxy presents an ambiguous morphology. It exhibits a relatively smooth overall structure, with a somewhat elliptical shape but it may be undergoing a merger or experiencing some other form of significant gravitational interaction. There appears to be two distinct luminous concentrations embedded within a fainter, more diffuse halo of light. One concentration is characterized by a reddish hue, while the other appears more blue-green, suggesting differing stellar populations or dust content. These concentrations might represent the remnant cores of merging galaxies, or potentially regions of enhanced star formation. The possibility of this being a relatively undisturbed elliptical galaxy cannot be ruled out, but the dual core structure warrants further investigation into its dynamical state. It does not appear to be a classic spiral galaxy due to the absence of clearly defined spiral arms.
