The galaxy exhibits an elliptical morphology. It appears largely smooth and lacks prominent spiral arm structures. The light distribution shows a centrally concentrated bulge, surrounded by a fainter, more diffuse halo. The central region presents a yellowish-white hue, possibly indicating an older stellar population. The outer regions exhibit a slightly bluer color, suggesting the presence of some younger stars, although the overall rate of star formation appears low. The shape is more disk-like and less spherical, resembling a flattened spheroid. There is no strong evidence of tidal features or recent merger activity.
