This galaxy appears as a relatively compact object with a smooth, elliptical morphology. The galaxy exhibits a dominant central bulge, appearing nearly round in shape. There are some irregularities present, which could suggest minor disturbances or tidal interactions.

The color gradient across the galaxy reveals a radial trend. The central region exhibits a more pronounced concentration of older stellar populations, indicated by a redder hue. The outer regions show a subtle shift towards bluer colors, suggesting the presence of younger stars.

Considering the overall smoothness and colour distribution, it seems likely we are observing a relatively massive galaxy with a relatively low star-formation rate.
