The galaxy appears as a centrally concentrated object with a smooth light distribution. It has an elliptical morphology, appearing significantly elongated rather than circular. There is a clear central bulge with a high concentration of light. The outer regions fade gradually into the background, with no distinct spiral arms or obvious features visible. There may be a very slight warp or asymmetry present, but it is subtle and not a dominant characteristic. The overall color is bluish-green, potentially indicating the presence of relatively young, hot stars or ionized gas. No strong tidal features or evidence of a major ongoing merger are apparent.
