The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. A bright, yellowish core dominates the central region, suggesting a significant population of older stars. The light gradually fades outwards from the core into a less defined halo, appearing bluish in color. This outer region could indicate some degree of ongoing or recent star formation activity, although it is not pronounced. There is no evidence of a distinct disk structure or spiral arms. Additionally, there are no obvious signs of a recent major merger or significant tidal disturbance. The overall appearance suggests a galaxy that is fairly evolved, likely with a substantial stellar mass and relatively low specific star formation rate.
