The galaxy presents an elliptical morphology, appearing elongated with a distinct central bulge. The bulge exhibits a concentrated, bright yellowish hue, suggesting a population of older stars. The outer regions of the galaxy display a more diffuse and bluish tinge, potentially indicating the presence of younger stellar populations or ongoing star formation. The galaxy appears relatively smooth, with no clear signs of spiral arms or significant dust lanes visible in this image. The overall structure suggests a relatively evolved system with a moderate degree of star formation occurring within its disk. There is a slight suggestion of tidal disturbances or minor interactions, but more detailed imaging is needed to confirm this hypothesis.
