The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears elliptical in shape, exhibiting a moderately luminous core that gradually fades into its surrounding halo. While the majority of the galaxy is smooth, hints of faint, diffuse features or a disk-like structure can be seen. These features suggest ongoing or past gravitational interactions, or perhaps residual spiral arms that are in the process of being disrupted. There is no obvious indication of a major ongoing merger event, with most of the galaxy's light appearing to originate from a single, coherent system. The overall color is characteristic of an older stellar population, dominated by redder wavelengths.
