The galaxy appears as a centrally concentrated, relatively smooth structure. It exhibits an elliptical morphology, with an overall rounded shape, though not perfectly spherical. There is little indication of spiral arms or a prominent disk component within the resolution constraints of the image. The light profile suggests a dominant bulge.  The galaxy shows a single core, without any obvious signs of tidal tails or merger features. The color is fairly uniform across the galaxy, suggestive of an older stellar population. The galaxy appears to be relatively isolated.
