The galaxy presents as a singular, centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape, displaying a high degree of roundness with no discernible disk features. Its core presents a bright yellow hue that gradually fades towards the outer regions of the galaxy. The galaxy lacks any clear spiral arm structures or significant dust lane obstructions. Faint hints of greenish color are visible within the galaxy's halo. There is no visual evidence of ongoing major merging activity, though minor disturbances or tidal features cannot be entirely ruled out due to the image's resolution. Overall, the galaxy appears to be a relatively evolved system, likely containing an older stellar population with a low star formation rate.
