The galaxy presents as a relatively smooth, round object. Its color profile indicates a significant population of older stars. Little to no structural features are discernible, suggesting an elliptical morphology. There is no evidence of spiral arms or a prominent disk. The galaxy appears isolated, with no obvious signs of ongoing or recent merger activity or tidal disturbances. The light is fairly uniform across the galaxy, with a slight central concentration that implies the presence of a dense core. The galaxy is at a distance where we can approximate its size to be around 4 kpc. There is little evidence of ongoing star formation.
