The galaxy exhibits an overall elliptical morphology, with an approximate aspect ratio suggesting a moderate degree of ellipticity. A smooth light profile is observed, lacking prominent spiral arms or bar structures. There appears to be a slight color gradient across the galaxy's body, transitioning from bluer hues towards one edge to redder hues towards the opposite edge and center, indicative of potential variations in stellar populations or dust distribution.  The galaxy appears to have some minor structural disturbances indicating that there could be a minor merger or tidal interaction occurring. The core of the galaxy exhibits a somewhat concentrated luminosity. The light is most likely being affected by dust or star formation.
