The galaxy presents as a centrally concentrated elliptical morphology. It displays a smooth, relatively featureless appearance, lacking prominent spiral arms or dust lanes. The core region exhibits a bright, concentrated luminosity, gradually diminishing towards the outer regions. The galaxy appears slightly elongated with a subtle flattening, as opposed to perfectly spherical. Color gradients indicate a redder hue in the central regions, suggesting an older stellar population, transitioning towards slightly bluer tones in the outskirts which could imply the presence of some younger stars, however, the dominant color is red. There's no visual evidence of any major ongoing merger events, though subtle disturbances cannot be ruled out at this resolution. The galaxy's profile seems to be consistent with a high Sersic index, suggesting a centrally concentrated light distribution.
