The galaxy presents a primarily smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, indicative of a significant stellar density, possibly a supermassive black hole at its center. The overall color profile skews toward the redder end of the spectrum, which suggests an older stellar population with minimal ongoing star formation. There is evidence of a subtle extended structure on one side that has a bluer color, possibly from a tidal interaction or minor merger event. This structure has relatively low surface brightness and a smooth appearance. The galaxy appears generally isolated.
