The galaxy presents as a moderately bright, elliptical-like system, exhibiting a concentrated central bulge. The light profile appears smooth, lacking distinct spiral arm structures or prominent dust lanes. The overall color suggests a relatively evolved stellar population, trending towards redder hues, particularly within the central region, which could indicate older stars. The outer regions of the galaxy appear slightly bluer, suggesting the possibility of some younger stars. The galaxy appears somewhat flattened, with a slight elongation. There is no obvious active galactic nucleus activity discernible from the image alone. Based on its smooth morphology, and evolved stellar population it could be an elliptical or lenticular galaxy.
