The galaxy appears as a relatively smooth, elliptical-shaped structure with a concentrated central bulge. Its color suggests an older stellar population, with a yellowish-red hue dominating the light emitted. There is no obvious evidence of ongoing, significant star formation, as indicated by the lack of prominent blue regions or spiral arms. The galaxy does not show any signs of major disturbances or merging activity; it has a generally relaxed morphology. It displays a predominantly round appearance and appears to be a quite massive galaxy.
