The galaxy presents a largely smooth, elliptical morphology, exhibiting a somewhat elongated shape. Its central region is dominated by a bright, concentrated core, suggesting a high stellar density. Moving outward from the core, the light intensity gradually decreases, with no apparent spiral arm structure or distinct features. A subtle color gradient is observed, with the central core displaying a warmer, yellowish hue, possibly indicating an older stellar population. The outer regions appear slightly bluer, hinting at the presence of younger stars, although this is not very pronounced. There are indications of a very slight disturbance or asymmetry in the overall structure, although this could be due to minor tidal interactions or intrinsic dynamics. Overall, this galaxy appears to be an evolved system dominated by older stellar populations, showing minimal ongoing star formation activity.
