The galaxy presents as a centrally concentrated, elliptical-like structure. Its light profile appears relatively smooth, with a bright, compact core that gradually diffuses outwards into a fainter, extended halo. The dominant color is a warm yellow-orange, suggesting an older stellar population within the core. There's a subtle color gradient as one moves outwards from the center, with hints of blue-green tones in the outer regions of the halo, potentially indicating the presence of younger, star-forming regions, albeit at a seemingly low rate. There's no apparent spiral arm structure or a distinct disk; the light distribution seems more spheroidal. No significant signs of tidal disturbances or ongoing mergers are immediately evident in the image. The galaxy appears to be an isolated system in a relatively relaxed state.
