The galaxy presents as a predominantly smooth, elliptical structure with a concentrated central bulge. Its color profile suggests an older stellar population, with a yellowish-red hue indicative of evolved stars. The galaxy exhibits a high degree of roundness in its overall shape. There's no obvious disk structure or spiral arm morphology, and no apparent major merger is occurring. Substructure within the galaxy is not evident, but a minor disturbance or interaction cannot be ruled out with the available image resolution. The galaxy appears to be relatively isolated and is not strongly interacting with its environment.
