The galaxy presents as a moderately luminous, elongated structure with a smooth, featureless appearance. The light profile suggests an elliptical morphology, potentially of type E4-E6 due to its notable ellipticity. The central region exhibits a higher concentration of light, gradually fading outwards towards the edges. The color appears to be generally yellow-orange, suggesting a relatively older stellar population with a lower rate of recent star formation. There is no apparent dust lane, spiral arm structure, or any sign of ongoing merger activity. It appears to be a relatively undisturbed, passively evolving system.
