The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There is an indication of a slightly elongated shape. The color profile is relatively uniform, displaying a moderate blue hue, indicative of possible ongoing or recent star formation activity. However, the smoothness of the light distribution suggests that the galaxy is dominated by an older stellar population, with star formation occurring at low levels. There are some suggestions of minor disturbances and a possible interacting system. Overall, the galaxy exhibits an intermediate morphology, falling somewhere between a pure elliptical and a disk galaxy with only weak structural features.
