The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region displays a yellow-orange hue, suggestive of an older stellar population dominating this area. Moving outwards from the core, the galaxy exhibits a gradual transition to a greenish-yellow tint in the outer regions. This subtle color shift might indicate the presence of a younger stellar population or ongoing low levels of star formation in these areas. There's no apparent spiral structure or prominent dust lanes. No significant tidal disturbances or interactions with neighboring galaxies are evident, implying a relatively isolated and dynamically stable system. The overall roundness indicates this object is most likely an elliptical galaxy, likely of significant mass.
