The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting characteristics that are more consistent with an elliptical morphology than a spiral. The light profile appears diffuse, lacking sharply defined spiral arms or a prominent disk structure. The galaxy is nearly round. There is a very slight indication of some tidal interactions or minor disturbances, but the overall structure remains largely undisturbed. The color distribution appears relatively uniform across the galaxy, with a slight central concentration that appears yellowish or redder in color, indicative of an older stellar population. There may be an additional object or disturbance on one side of the galaxy. The galaxy appears to have a mass just above 10^9 solar masses. The rate of star formation is slow.
