The galaxy presents as a predominantly smooth, elliptical structure with a concentrated central bulge. The light profile appears largely featureless, lacking prominent spiral arms or distinct dust lanes. There is a slight elongation, however the galaxy is mostly round. The core displays a yellowish hue, transitioning outwards to a more diffuse, bluish halo. The color gradient suggests a mix of stellar populations, with the core potentially dominated by older, redder stars, while the halo may contain a younger, bluer population or exhibit evidence of ongoing star formation. There's no visual evidence of a major ongoing merger or significant tidal disturbances.
