The galaxy presents as a single, concentrated luminosity with a near-spherical morphology. The color profile appears slightly redder, indicating an older stellar population with relatively little ongoing star formation activity. There is no discernible disk structure or spiral arm presence. No signs of active galactic nuclei or significant dust lanes are apparent within the resolution of the image. The absence of significant tidal features or close companion galaxies suggests the galaxy is not currently undergoing a major merger event. Overall, the galaxy seems to be a fairly massive, relaxed system, likely an elliptical or lenticular galaxy that is not forming many stars.