The galaxy appears as a relatively compact object, exhibiting a somewhat elongated shape, suggesting an elliptical morphology or a disk galaxy viewed at an angle. The galaxy's light is predominantly smooth, indicative of an older stellar population with minimal dust obscuration. There is a subtle color gradient, transitioning from a slightly bluer hue in what might be its outer regions to a redder color towards the center. This may indicate some ongoing, albeit low-level, star formation in the galaxy's periphery, or varying stellar populations throughout. The overall appearance is indicative of a system that is not undergoing significant mergers or major disturbances.
