The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The light profile is concentrated towards the center, with a gradual decrease in intensity outwards. The core exhibits a yellowish hue, possibly indicating an older stellar population. A slight color gradient suggests the presence of some younger, bluer stars towards the outer regions, though the dominant color remains in the redder part of the spectrum. There is no distinct evidence of spiral arms or a prominent disk structure. There are no obvious signs of significant tidal disturbances or ongoing major mergers. The galaxy appears relatively undisturbed and evolved.
