The galaxy appears to be an elliptical morphology. The light is concentrated in a central bulge, with a smooth light distribution indicating an older stellar population. The galaxy has a yellow/orange color, indicating minimal ongoing star formation. The elongation suggests that it may be a E4-E6 galaxy. This galaxy also shows signs of potentially having a minor disturbance, perhaps related to a potential recent or ongoing merger, but the tidal features are not very prominent. The roundness is visible, but more like a less pronounced disk galaxy. The presence of a possible companion object and some disrupted features could mean that there is ongoing dynamical activity or a merger with a smaller galaxy.