The galaxy presents as an elliptical or lenticular morphology. The object has a smooth appearance without prominent spiral arms or a distinct disk structure. The galaxy's shape is somewhat elongated, displaying a deviation from perfect circularity, but not dramatically so. There is little evidence of ongoing mergers or major disturbances in its structure. Its color is generally consistent with an older stellar population, lacking bright blue regions indicative of recent, intense star formation. The relatively low star formation rate is further supported by its reddish hue. The galaxy’s mass falls within the range expected for a typical elliptical galaxy.
