This galaxy exhibits an elliptical morphology, appearing as a relatively smooth, concentrated distribution of light. A slight elongation is visible, though it is generally rounded in shape. The galaxy appears to be undergoing a merging event, with a secondary object in close proximity. The system exhibits a degree of disturbance, suggesting gravitational interaction. The central region is characterized by a bright, compact core, indicative of a significant concentration of stars. Color gradients suggest an aging stellar population within the primary galaxy, with a blueish tint on one side. Overall, the object is moderately luminous and relatively massive.
