The galaxy presents as a relatively smooth, centrally concentrated elliptical galaxy with a dominant bulge. Its shape is generally round. The core exhibits a bright yellowish-white hue, indicating a high density of older stars. The color of the core suggests the presence of an older stellar population. There is little to no visible dust lane or active star formation regions in this galaxy. The galaxy does not appear to be undergoing any major merging events or displaying significant tidal disturbances, maintaining a fairly regular elliptical morphology.
