The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated luminosity, suggesting a significant stellar population. The light profile appears centrally concentrated, fading gradually outward, lacking distinct spiral arm features. The overall color is yellowish, indicative of an older stellar population with a lower rate of current star formation. There is no visually apparent evidence of major mergers or tidal disturbances. The galaxy appears relatively isolated within the observed field, with no immediately interacting companions.
