The galaxy presents an elliptical morphology, displaying a smooth, relatively featureless structure. A concentrated central bulge is visible, emitting a yellowish-white light, suggestive of an older stellar population. The galaxy's outer regions fade gradually into the background, displaying a bluish hue which might indicate ongoing, albeit low-level, star formation activity within the galaxy's disk. The overall shape appears mostly round. There's no evidence of strong tidal disturbances or major merger activity affecting the galaxy's structure.
