The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features suggestive of recent mergers or tidal interactions. The core region exhibits a bright, concentrated luminosity, decreasing gradually outwards toward the galaxy's periphery. The overall color is consistent with an older stellar population, showing a slight bluer hue due to possible intermediate age stars in the galaxy. The apparent flattening and elongation of the galaxy indicate it is an elliptical galaxy.
