The galaxy appears as a moderately bright, lenticular or early-type spiral galaxy. The central bulge exhibits a yellow-orange hue, suggesting an older stellar population. Surrounding the bulge is a faint, flattened disk with a bluish tint, indicating the presence of younger, hotter stars and potential ongoing star formation. The galaxy demonstrates an overall smooth morphology with a hint of a disk, but with only minor structural irregularities or disturbances observed. Its shape is somewhat elongated. No clear signs of a major merger or strong tidal interactions are apparent.
