The galaxy presents as a relatively compact, elliptical or lenticular system. Its light is dominated by older stellar populations, indicated by the yellowish-white color of its central region. The surface brightness profile appears to be smooth, with a gradual decline in intensity from the core outward, suggesting a well-mixed distribution of stars. There are no apparent spiral arms or prominent dust lanes visible in this imaging. The galaxy appears to be isolated, with no clear signs of tidal interactions or recent merger events evident in the surrounding environment.
