The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge that gradually fades into an extended halo. The galaxy displays a mild elongation, suggesting a deviation from a perfectly spherical shape. The color profile indicates a population of primarily older stars, with a slightly redder hue observed in the outer regions, possibly due to a higher concentration of dust or a change in stellar population. There is a slight suggestion of disturbed morphology which could be a tidal tail on the right side. There is no readily apparent spiral structure or distinct star-forming regions discernible in this image, though some low levels of star formation may be ongoing based on luminosity. Overall, the galaxy seems to be a relatively quiescent system, typical of early-type galaxies observed at its redshift.
