The galaxy presents as a centrally concentrated, smooth object. It appears elliptical in shape, exhibiting a high degree of radial symmetry. The galaxy's color is predominantly yellowish-white, suggesting an older stellar population. There is no obvious spiral arm structure or dust lane obscuration visible, indicating a relative lack of ongoing star formation. The surface brightness profile appears to decrease smoothly from the center outwards, with no distinct features or abrupt changes in gradient. There is no apparent interaction with neighboring galaxies, and the overall morphology suggests it is a relatively isolated system.
