This galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a relatively high degree of roundness.  There's a noticeable color gradient; the central region exhibits a yellow-orange hue, which suggests a population of older stars. Moving outwards, the color shifts towards a redder, more diffuse halo. No prominent spiral arms or disk-like structure are discernible. There is no evidence of any major merger activity or significant tidal disturbances. The light profile indicates a substantial stellar mass. The star formation rate appears to be relatively low, suggesting a quiescent galaxy with a primarily evolved stellar population.
