The galaxy presents an elliptical morphology, with a smooth light distribution characterized by a concentrated central bulge. It appears yellowish-orange in color, suggesting a stellar population dominated by older, redder stars. The overall form is somewhat elongated. There's a subtle presence of bluer light in the galaxy's outer regions. There is no sign of spiral arms or a prominent disk structure. Evidence suggests minimal disturbances from mergers. The image indicates the galaxy is a relatively massive system.
