The galaxy presents as a single, moderately bright object with a smooth, elliptical morphology. Its color appears predominantly yellow-orange, suggesting an older stellar population with a reduced rate of star formation. The overall structure lacks any distinct spiral arms or bar features. There is no indication of a major ongoing merger, although subtle asymmetries within the light distribution cannot be completely ruled out given the image resolution. The galaxy's round appearance points towards a possible E0-E3 classification on the Hubble sequence.
