The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated towards the center. It exhibits a dominant bulge component with a noticeable absence of spiral arm structures. The galaxy displays a gradient in color, with a slightly bluer core transitioning to redder hues in the outer regions. This suggests a central population of younger, hotter stars possibly caused by high star formation rate, surrounded by an older stellar population. There's a slight asymmetry in the shape, possibly hinting at tidal interactions or minor disturbances although no distinct signs of merging are visible. Overall, the galaxy appears to be a quiescent system likely in the process of transitioning to a red and dead galaxy with a low star formation rate.
