The galaxy presents an elliptical morphology, appearing mostly smooth with a concentrated central bulge. The light distribution suggests a gradual decrease in brightness from the core outwards, lacking any distinct spiral arm features. There is a slight asymmetry in the outer regions, potentially hinting at a minor interaction or internal disturbance. The galaxy exhibits a yellow-red hue, possibly indicating an older stellar population and/or dust obscuration within the system. Overall, the galaxy appears to be a relatively evolved system, possibly undergoing transformation processes.
