The galaxy presents as a somewhat elongated structure. The galaxy's color appears to be primarily yellowish-white, with a slightly brighter, more concentrated core, potentially suggesting an older stellar population in the central region. The disk appears to be relatively smooth. Faint blue-ish regions are observed around the perimeter, possibly indicative of younger stars or ongoing star formation. There is no pronounced spiral structure visible. The galaxy seems to be relatively undisturbed, with no strong signs of a major merger event. It is generally smooth with some possible minor disturbance.