The galaxy presents as a single, relatively smooth object. The light is concentrated towards the center and gradually fades towards the edges. There is very little evidence of substructure within the galaxy; spiral arms are not detectable, and the overall structure appears largely spheroidal. The color appears fairly uniform across the galaxy, with a slight red hue, indicating an older stellar population. The galaxy appears isolated, with no other nearby galaxies suggesting a potential interaction or ongoing merger. Based on its appearance, the galaxy is likely an elliptical or lenticular type galaxy, with a dominant spheroidal component and minimal ongoing star formation.
