The galaxy appears as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical type, with a high degree of symmetry. The light distribution is dominated by a central bulge, which presents a yellowish hue, likely indicating an older stellar population. Fainter bluish regions are observed in the outer areas, suggesting the presence of some younger, hotter stars, but the smooth appearance indicates these are not organized into spiral arms. There is no evidence of strong tidal features or morphological disturbances, and the galaxy looks relatively isolated and unperturbed. The absence of strong dust lanes or distinct structures further reinforces the assessment of a relatively passive elliptical galaxy. The general roundness indicates a nearly face-on orientation.
