The galaxy appears as a slightly elongated, moderately bright object with a smooth light distribution. Its color is predominantly a yellow-orange hue, possibly indicating an older stellar population with fewer young, hot stars. There is a subtle color gradient, transitioning from a slightly bluer tint towards the edges to a slightly more reddish color towards the core. No distinct spiral arms or dust lanes are discernible. The overall morphology suggests a galaxy that could be an elliptical or possibly a lenticular type, exhibiting characteristics of a relatively evolved system. There is also a slight chance that the galaxy is undergoing a merger or has some sort of tidal disturbance.
