The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a high degree of luminosity. The color profile indicates a dominant population of older stars, suggested by the redder hue in the galaxy's central region which may be a sign of little to no current star formation. There is a hint of a faint disk surrounding the bulge. The galaxy does not show any obvious signs of strong tidal interactions or major disturbances.
