The galaxy presents as a relatively compact object with a generally smooth morphology. Its overall shape approximates a circular form. However, there appears to be evidence of potential tidal disturbances or interactions. There are some faint wisps of diffuse material extending outwards in what may be minor disturbance that could be indicative of recent merger activity or gravitational interaction with another nearby galaxy. The galaxy appears to be relatively undisturbed, though the minor disturbances may be more indicative of merging. The galaxy is not elongated.
