The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. There are no distinct spiral arms or a prominent disk component visible. The galaxy exhibits a general yellowish-white color across its entirety, suggesting an older stellar population with limited ongoing star formation. There is no apparent dust obscuration or significant features indicative of recent merger activity, such as tidal tails or distorted morphology, with an essentially round, non-elongated shape. The overall appearance suggests this is a relatively massive and evolved galaxy, located at a considerable distance.
